. . . . . . "Una kilonova (tambi\u00E9n llamada macronova o proceso de supernova de tipo r) ocurre cuando dos estrellas de neutrones o una estrella de neutrones y un agujero negro se fusionan a partir de un sistema binario. Por lo general emiten fuertes se\u00F1ales de radiaci\u00F3n electromagn\u00E9tica debido al proceso de desintegraci\u00F3n de iones pesados que son producidos y expulsados de forma isotr\u00F3pica durante el proceso de fusi\u00F3n. Ser\u00EDa muy similar a una supernova, pero m\u00E1s corta y con menor emisi\u00F3n.\u200BUn tiempo antes de la fusi\u00F3n, ambos objetos compactos empiezan a rotar sobre el centro de masas del sistema binario muy r\u00E1pidamente, lo cual se teoriz\u00F3 que podr\u00EDa ser una fuente importante de ondas gravitacionales (GWs).\u200B En octubre de 2017 se pudo demostrar finalmente dicha teor\u00EDa mediante resultados experimentales. El observatorio de ondas gravitacionales LIGO y el observatorio Austral Europeo (ESO) anunciaron las primeras evidencias de una kilonova que hab\u00EDa emitido ondas gravitacionales. Tambi\u00E9n se cree que es origen de explosiones de rayos gamma de corta duraci\u00F3n y la fuente m\u00E1s predominante de elementos estables pesados en el universo. La primera detecci\u00F3n clara de una kilonova fue asociada con la explosi\u00F3n de rayos gamma de corta duraci\u00F3n GRB 130603B. Esta explosi\u00F3n de rayos gamma se produjo en una galaxia relativamente cercana, permitiendo que la emisi\u00F3n infrarroja de la kilonova pudiera ser detectada utilizando el telescopio espacial Hubble. El 17 de agosto de 2017 el observatorio de ondas gravitacionales LIGO estadounidense y el proyecto VIRGO en Italia, captaron ondas gravitacionales en un punto determinado del espacio. Dos segundos despu\u00E9s dos observatorios de radiaci\u00F3n gamma percibieron una fuente en el cielo. A la ca\u00EDda de la noche se apuntaron varios observatorios para visualizar que hab\u00EDa sido el resplandor de radiaci\u00F3n gamma, en alg\u00FAn punto en la constelaci\u00F3n de la Hidra, descubri\u00E9ndose la fusi\u00F3n de dos estrellas de neutrones en una galaxia a 130 millones de a\u00F1os luz.\u200B"@es . . . "A kilonova (also called a macronova or r-process supernova) is a transient astronomical event that occurs in a compact binary system when two neutron stars or a neutron star and a black hole merge. Kilonovae are thought to emit short gamma-ray bursts and strong electromagnetic radiation due to the radioactive decay of heavy r-process nuclei that are produced and ejected fairly isotropically during the merger process."@en . . . "\u30AD\u30ED\u30CE\u30F4\u30A1"@ja . . . "\u041A\u0456\u043B\u043E\u043D\u043E\u0432\u0430 (\u0456\u043D\u0448\u0456 \u043D\u0430\u0437\u0432\u0438: \u043C\u0430\u043A\u0440\u043E\u043D\u043E\u0432\u0430, \u0441\u0443\u043F\u0435\u0440\u043D\u043E\u0432\u0430 r-\u043F\u0440\u043E\u0446\u0435\u0441\u0443) - \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0456\u0447\u043D\u0430 \u043F\u043E\u0434\u0456\u044F \u0437\u043B\u0438\u0442\u0442\u044F \u0434\u0432\u043E\u0445 \u043D\u0435\u0439\u0442\u0440\u043E\u043D\u043D\u0438\u0445 \u0437\u0456\u0440 \u0430\u0431\u043E \u043D\u0435\u0439\u0442\u0440\u043E\u043D\u043D\u043E\u0457 \u0437\u043E\u0440\u0456 \u0442\u0430 \u0447\u043E\u0440\u043D\u043E\u0457 \u0434\u0456\u0440\u0438. \u041F\u043E\u0434\u0456\u044F \u0441\u0443\u043F\u0440\u043E\u0432\u043E\u0434\u0436\u0443\u0454\u0442\u044C\u0441\u044F \u043F\u043E\u0442\u0443\u0436\u043D\u0438\u043C \u0435\u043B\u0435\u043A\u0442\u0440\u043E\u043C\u0430\u0433\u043D\u0456\u0442\u043D\u0438\u043C \u0432\u0438\u043F\u0440\u043E\u043C\u0456\u043D\u044E\u0432\u0430\u043D\u043D\u044F\u043C, \u043F\u043E\u0432'\u044F\u0437\u0430\u043D\u0438\u043C \u0456\u0437 \u0440\u043E\u0437\u043F\u0430\u0434\u043E\u043C \u044F\u0434\u0435\u0440 \u0432\u0430\u0436\u043A\u0438\u0445 \u0435\u043B\u0435\u043C\u0435\u043D\u0442\u0456\u0432, \u0449\u043E \u0443\u0442\u0432\u043E\u0440\u0438\u043B\u0438\u0441\u044F \u0432\u043D\u0430\u0441\u043B\u0456\u0434\u043E\u043A r-\u043F\u0440\u043E\u0446\u0435\u0441\u0456\u0432, \u044F\u043A\u0456 \u0432\u0456\u0434\u0431\u0443\u0432\u0430\u044E\u0442\u044C\u0441\u044F \u0443 \u043F\u0440\u0430\u043A\u0442\u0438\u0447\u043D\u043E \u0456\u0437\u043E\u0442\u0440\u043E\u043F\u043D\u0438\u0445 \u0432\u0438\u043A\u0438\u0434\u0430\u0445, \u0430\u043D\u0430\u043B\u043E\u0433\u0456\u0447\u043D\u043E \u0441\u043B\u0430\u0431\u043A\u0456\u0439 \u0441\u0443\u043F\u0435\u0440\u043D\u043E\u0432\u0456\u0439 \u0456\u0437 \u043A\u043E\u0440\u043E\u0442\u043A\u0438\u043C \u0447\u0430\u0441\u043E\u043C \u0436\u0438\u0442\u0442\u044F."@uk . . . "A kilonova (also called a macronova or r-process supernova) is a transient astronomical event that occurs in a compact binary system when two neutron stars or a neutron star and a black hole merge. Kilonovae are thought to emit short gamma-ray bursts and strong electromagnetic radiation due to the radioactive decay of heavy r-process nuclei that are produced and ejected fairly isotropically during the merger process."@en . . . . . "Een kilonova (macronova of r-proces supernova) is een voorbijgaande astronomische gebeurtenis die zich voordoet in een compact binair systeem wanneer twee neutronensterren of een neutronenster en een zwart gat in elkaar opgaan. Kilonovae worden gedacht korte gammaflitsen en sterke elektromagnetische straling uit te zenden door het radioactief verval van zware r-proces kernen die tijdens het fusieproces vrij isotropisch worden geproduceerd en uitgeworpen. De eerste kilonova werd waargenomen in 2013 met behulp van de ruimtetelescoop Hubble."@nl . "Kilonova"@it . . . . "\u0645\u0633\u062A\u0639\u0631 \u0645\u0627\u0643\u0631\u0648"@ar . "\u5343\u65B0\u661F\uFF08kilonova \u6216 r-process \u8D85\u65B0\u661F\uFF09\uFF0C\u662F\u4E00\u7C7B\u53D1\u751F\u4E8E\u53CC\u81F4\u5BC6\u5929\u4F53\uFF08\u5982\u53CC\u4E2D\u5B50\u661F\uFF0C\u4E2D\u5B50\u661F\u4E0E\u9ED1\u6D1E\uFF09\u5E76\u5408\u8FC7\u7A0B\u4E2D\u7684\u6682\u73B0\u5929\u6587\u4E8B\u4EF6\u3002\u7531\u4E8E\u5728\u5E76\u5408\u8FC7\u7A0B\u4E2D\u4EA7\u751F\u5404\u5411\u540C\u6027\u7684\u7269\u8D28\u629B\u5C04\u548C\u91CD\u7684R-\u904E\u7A0B\u5143\u7D20\u7684\u653E\u5C04\u6027\u8870\u53D8\uFF0C\u5343\u65B0\u661F\u88AB\u8BA4\u4E3A\u53EF\u4EE5\u53D1\u51FA\u77ED\u4F3D\u739B\u5C04\u7EBF\u66B4\u548C\u5F3A\u7535\u78C1\u8F90\u5C04\u3002 \u4EBA\u7C7B\u5229\u7528\u54C8\u52C3\u7A7A\u95F4\u671B\u8FDC\u955C\u4E8E2013\u5E74\u9996\u6B21\u89C2\u6D4B\u5230\u5343\u65B0\u661F\u4E8B\u4EF6\u3002"@zh . . "\u041A\u0456\u043B\u043E\u043D\u043E\u0432\u0430"@uk . "\u5343\u65B0\u661F\uFF08kilonova \u6216 r-process \u8D85\u65B0\u661F\uFF09\uFF0C\u662F\u4E00\u7C7B\u53D1\u751F\u4E8E\u53CC\u81F4\u5BC6\u5929\u4F53\uFF08\u5982\u53CC\u4E2D\u5B50\u661F\uFF0C\u4E2D\u5B50\u661F\u4E0E\u9ED1\u6D1E\uFF09\u5E76\u5408\u8FC7\u7A0B\u4E2D\u7684\u6682\u73B0\u5929\u6587\u4E8B\u4EF6\u3002\u7531\u4E8E\u5728\u5E76\u5408\u8FC7\u7A0B\u4E2D\u4EA7\u751F\u5404\u5411\u540C\u6027\u7684\u7269\u8D28\u629B\u5C04\u548C\u91CD\u7684R-\u904E\u7A0B\u5143\u7D20\u7684\u653E\u5C04\u6027\u8870\u53D8\uFF0C\u5343\u65B0\u661F\u88AB\u8BA4\u4E3A\u53EF\u4EE5\u53D1\u51FA\u77ED\u4F3D\u739B\u5C04\u7EBF\u66B4\u548C\u5F3A\u7535\u78C1\u8F90\u5C04\u3002 \u4EBA\u7C7B\u5229\u7528\u54C8\u52C3\u7A7A\u95F4\u671B\u8FDC\u955C\u4E8E2013\u5E74\u9996\u6B21\u89C2\u6D4B\u5230\u5343\u65B0\u661F\u4E8B\u4EF6\u3002"@zh . "Una kilonova \u00E8 una esplosione astronomica che si verifica quando due oggetti celesti superdensi, come stelle di neutroni e buchi neri, si fondono tra loro. La loro luminosit\u00E0 \u00E8 1000 volte pi\u00F9 intensa di quella di una stella nova e da 1/10 a 1/100 di quella di una supernova. Lo spettro energetico di una kilonova \u00E8 concentrato prevalentemente nella zona dell'infrarosso vicino, a causa dell'elevata produzione di elementi radioattivi pesanti e ricchi di neutroni che fungerebbero da \"filtro\" alle radiazioni con frequenze pi\u00F9 elevate."@it . . "Kilonova"@nl . "\u041A\u0456\u043B\u043E\u043D\u043E\u0432\u0430 (\u0456\u043D\u0448\u0456 \u043D\u0430\u0437\u0432\u0438: \u043C\u0430\u043A\u0440\u043E\u043D\u043E\u0432\u0430, \u0441\u0443\u043F\u0435\u0440\u043D\u043E\u0432\u0430 r-\u043F\u0440\u043E\u0446\u0435\u0441\u0443) - \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0456\u0447\u043D\u0430 \u043F\u043E\u0434\u0456\u044F \u0437\u043B\u0438\u0442\u0442\u044F \u0434\u0432\u043E\u0445 \u043D\u0435\u0439\u0442\u0440\u043E\u043D\u043D\u0438\u0445 \u0437\u0456\u0440 \u0430\u0431\u043E \u043D\u0435\u0439\u0442\u0440\u043E\u043D\u043D\u043E\u0457 \u0437\u043E\u0440\u0456 \u0442\u0430 \u0447\u043E\u0440\u043D\u043E\u0457 \u0434\u0456\u0440\u0438. \u041F\u043E\u0434\u0456\u044F \u0441\u0443\u043F\u0440\u043E\u0432\u043E\u0434\u0436\u0443\u0454\u0442\u044C\u0441\u044F \u043F\u043E\u0442\u0443\u0436\u043D\u0438\u043C \u0435\u043B\u0435\u043A\u0442\u0440\u043E\u043C\u0430\u0433\u043D\u0456\u0442\u043D\u0438\u043C \u0432\u0438\u043F\u0440\u043E\u043C\u0456\u043D\u044E\u0432\u0430\u043D\u043D\u044F\u043C, \u043F\u043E\u0432'\u044F\u0437\u0430\u043D\u0438\u043C \u0456\u0437 \u0440\u043E\u0437\u043F\u0430\u0434\u043E\u043C \u044F\u0434\u0435\u0440 \u0432\u0430\u0436\u043A\u0438\u0445 \u0435\u043B\u0435\u043C\u0435\u043D\u0442\u0456\u0432, \u0449\u043E \u0443\u0442\u0432\u043E\u0440\u0438\u043B\u0438\u0441\u044F \u0432\u043D\u0430\u0441\u043B\u0456\u0434\u043E\u043A r-\u043F\u0440\u043E\u0446\u0435\u0441\u0456\u0432, \u044F\u043A\u0456 \u0432\u0456\u0434\u0431\u0443\u0432\u0430\u044E\u0442\u044C\u0441\u044F \u0443 \u043F\u0440\u0430\u043A\u0442\u0438\u0447\u043D\u043E \u0456\u0437\u043E\u0442\u0440\u043E\u043F\u043D\u0438\u0445 \u0432\u0438\u043A\u0438\u0434\u0430\u0445, \u0430\u043D\u0430\u043B\u043E\u0433\u0456\u0447\u043D\u043E \u0441\u043B\u0430\u0431\u043A\u0456\u0439 \u0441\u0443\u043F\u0435\u0440\u043D\u043E\u0432\u0456\u0439 \u0456\u0437 \u043A\u043E\u0440\u043E\u0442\u043A\u0438\u043C \u0447\u0430\u0441\u043E\u043C \u0436\u0438\u0442\u0442\u044F."@uk . "Kilonova"@es . . . "\uD0AC\uB85C\uB178\uBC14(kilonova)\uB294 \uC911\uC131\uC790\uBCC4 \uC30D\uC774\uB098 \uC911\uC131\uC790\uBCC4\uACFC \uBE14\uB799\uD640\uB85C \uC774\uB8E8\uC5B4\uC9C4 \uC5F0\uC131\uACC4\uC5D0\uC11C \uB450 \uCC9C\uCCB4\uAC00 \uCDA9\uB3CC\uD560 \uB54C \uC77C\uC5B4\uB098\uB294 \uC21C\uAC04\uC801\uC778 \uD604\uC0C1\uC73C\uB85C, \uB9E4\uD06C\uB85C\uB178\uBC14(macronova)\uB098 R-\uACFC\uC815 \uCD08\uC2E0\uC131(r-process supernova)\uC774\uB77C\uACE0\uB3C4 \uD55C\uB2E4. \uD0AC\uB85C\uB178\uBC14\uB294 \uBB34\uAC70\uC6B4 R-\uACFC\uC815 \uD575\uC774 \uB4F1\uBC29\uC801\uC73C\uB85C \uBC29\uC0AC\uC131 \uBD95\uAD34\uD558\uC5EC \uC9E7\uC740 \uAC10\uB9C8\uC120 \uD3ED\uBC1C\uC744 \uC77C\uC73C\uD0AC \uAC83\uC774\uB77C\uACE0 \uC5EC\uACA8\uC9C4\uB2E4. \uD0AC\uB85C\uB178\uBC14\uB77C\uB294 \uC6A9\uC5B4\uB294 \uD0AC\uB85C\uB178\uBC14\uC758 \uCD5C\uACE0 \uBC1D\uAE30\uAC00 \uC77C\uBC18\uC801\uC778 \uC2E0\uC131(\uB178\uBC14)\uC758 1000\uBC30 \uC815\uB3C4\uB77C\uB294 \uC810\uC5D0\uC11C \uC81C\uC548\uB418\uC5C8\uC73C\uBA70, \uC774\uB294 \uC77C\uBC18\uC801\uC778 \uCD08\uC2E0\uC131 \uBC1D\uAE30\uC758 10~100\uBC30 \uC815\uB3C4\uC774\uB2E4. \uCD5C\uCD08\uB85C \uBC1C\uACAC\uB41C \uD0AC\uB85C\uB178\uBC14\uB294 \uAC10\uB9C8\uC120 \uD3ED\uBC1C SGRB 130603B\uB85C, \uC2A4\uC704\uD504\uD2B8 \uAC10\uB9C8\uC120 \uD3ED\uBC1C \uC784\uBB34, WIND, \uD5C8\uBE14 \uC6B0\uC8FC \uB9DD\uC6D0\uACBD\uC744 \uD1B5\uD574 \uAD00\uCE21\uD558\uC600\uB2E4. 2018\uB144 10\uC6D4, 2015\uB144 \uBC1C\uACAC\uB41C \uAC10\uB9C8\uC120 \uD3ED\uBC1C \uAC00 2017\uB144 \uBC1C\uACAC\uB41C \uC911\uB825\uD30C \uACFC \uC720\uC0AC\uD55C \uD604\uC0C1\uC774\uB77C\uB294 \uC8FC\uC7A5\uC774 \uC81C\uAE30\uB418\uC5C8\uB2E4. \uB2E4\uC591\uD55C \uC804\uC790\uAE30\uD30C\uB85C \uAD00\uCE21\uD55C \uBAA8\uC2B5\uC774\uB098 \uD604\uC0C1\uC774 \uC77C\uC5B4\uB09C \uC740\uD558\uC758 \uD658\uACBD \uB4F1\uC774 \uB9E4\uC6B0 \uC720\uC0AC\uD558\uC5EC \uBCC4\uAC1C\uC758 \uC0AC\uAC74\uCC98\uB7FC \uBCF4\uC774\uB294 \uB450 \uD604\uC0C1\uC774 \uC0AC\uC2E4\uC740 \uC911\uC131\uC790\uBCC4\uC758 \uCDA9\uB3CC\uC774\uB77C\uB294 \uAC19\uC740 \uC6D0\uC778\uC73C\uB85C \uC77C\uC5B4\uB09C \uC0AC\uAC74\uC73C\uB85C, \uB458 \uBAA8\uB450 \uD0AC\uB85C\uB178\uBC14\uC758 \uACFC\uB3C4\uC801\uC778 \uC0C1\uD0DC\uB77C\uB294 \uAC83\uC73C\uB85C, \uC774 \uC8FC\uC7A5\uC774 \uB9DE\uB2E4\uBA74 \uAE30\uC874\uC5D0 \uCD94\uC815\uB418\uC5C8\uB358 \uAC83\uBCF4\uB2E4 \uD0AC\uB85C\uB178\uBC14\uB294 \uC0C1\uB2F9\uD788 \uD754\uD55C \uD604\uC0C1\uC73C\uB85C \uC608\uCE21\uB41C\uB2E4."@ko . . "Uma kilonova (tamb\u00E9m chamada de uma 'macronova' ou uma 'supernova de processo-r\") ocorre quando duas estrelas de n\u00EAutrons ou uma estrela de n\u00EAutron e um buraco negro se unem em um sistema bin\u00E1rio. Uma forte radia\u00E7\u00E3o eletromagn\u00E9tica \u00E9 emitida devido ao decaimento de \u00EDons do pesado processo-r que s\u00E3o produzidos e ejetados basicamente na forma isotr\u00F3pica durante o processo de fus\u00E3o \u2014 semelhante a uma supernova fraca e de curta dura\u00E7\u00E3o.O espiral e a fus\u00E3o dos dois objetos compactos s\u00E3o uma forte fonte de ondas gravitacionais (GWs). Acredita-se que possa ser o emissor de curtas explos\u00F5es de raios gama e a fonte predominante do est\u00E1vel processo-r de elementos no Universo."@pt . . . "Kilonova je astronomick\u00E1 ud\u00E1lost, p\u0159i n\u00ED\u017E dojde ke splynut\u00ED dvou neutronov\u00FDch hv\u011Bzd nebo neutronov\u00E9 hv\u011Bzdy a \u010Dern\u00E9 d\u00EDry. Tento jev je p\u0159ibli\u017En\u011B 1000\u00D7 jasn\u011Bj\u0161\u00ED ne\u017E b\u011B\u017En\u00E1 nova \u2013 z toho vych\u00E1z\u00ED jej\u00ED n\u00E1zev. Kilonova se pova\u017Euje za jeden z pravd\u011Bpodobn\u00FDch zdroj\u016F gama z\u00E1blesk\u016F a siln\u00E9ho elektromagnetick\u00E9ho z\u00E1\u0159en\u00ED vznikaj\u00EDc\u00EDho v d\u016Fsledku radioaktivn\u00EDho rozpadu nov\u011B vznikl\u00FDch prvk\u016F."@cs . "Kilonova atau Makronova adalah peristiwa astronomi sementara yang terjadi ketika sepasang bintang neutron atau pasangan bintang neutron dan lubang hitam berinteraksi dan bertabrakan sehingga terjadi ledakan sinar gamma sesaat dengan kecerlangan 1000 kali dari nova tapi tidak secerah supernova. Penggabungan bintang neutron biner dapat mengguncang ruang-waktu, menghasilkan ledakan elektromagnetik paling kuat di alam semesta dan cahaya optik samar dari sinar gamma pendek hingga gelombang radio dari reaksi nuklir proses-r yang terjadi dari puing-puing tabrakan dan dikeluarkan secara isotropis selama proses penggabungan."@in . "Kilonova atau Makronova adalah peristiwa astronomi sementara yang terjadi ketika sepasang bintang neutron atau pasangan bintang neutron dan lubang hitam berinteraksi dan bertabrakan sehingga terjadi ledakan sinar gamma sesaat dengan kecerlangan 1000 kali dari nova tapi tidak secerah supernova. Penggabungan bintang neutron biner dapat mengguncang ruang-waktu, menghasilkan ledakan elektromagnetik paling kuat di alam semesta dan cahaya optik samar dari sinar gamma pendek hingga gelombang radio dari reaksi nuklir proses-r yang terjadi dari puing-puing tabrakan dan dikeluarkan secara isotropis selama proses penggabungan. Meskipun kecil kilonova akan terjadi di dekatnya dalam waktu dekat, kilonova terjadi 1.000 tahun cahaya dari Bumi sekarang (meskipun 80 juta tahun sebelum tata surya terbentuk yang mengunggulkan tata surya dengan unsur-unsur yang menyusun planet-planet saat ini). Kilonova dapat terjadi sedekat itu dengan Bumi setiap 100 juta tahun, perkiraan astrofisika. Jadi kita tidak mungkin melihatnya, tetapi beberapa mungkin telah terjadi selama 4,5 miliar tahun sejarah Bumi. Itu bisa menimbulkan konsekuensi yang menyakitkan bagi apa pun yang hidup di planet ini pada saat itu."@in . . . . "\u041A\u0438\u043B\u043E\u043D\u00F3\u0432\u0430\u044F (kilonova) \u2014 \u044D\u0442\u043E \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0438\u0447\u0435\u0441\u043A\u043E\u0435 \u0441\u043E\u0431\u044B\u0442\u0438\u0435, \u043F\u0440\u043E\u0438\u0441\u0445\u043E\u0434\u044F\u0449\u0435\u0435 \u0432 \u0434\u0432\u043E\u0439\u043D\u044B\u0445 \u0437\u0432\u0451\u0437\u0434\u043D\u044B\u0445 \u0441\u0438\u0441\u0442\u0435\u043C\u0430\u0445 \u043F\u0440\u0438 \u0441\u043B\u0438\u044F\u043D\u0438\u0438 \u0434\u0432\u0443\u0445 \u043D\u0435\u0439\u0442\u0440\u043E\u043D\u043D\u044B\u0445 \u0437\u0432\u0451\u0437\u0434 \u0438\u043B\u0438 \u043D\u0435\u0439\u0442\u0440\u043E\u043D\u043D\u043E\u0439 \u0437\u0432\u0435\u0437\u0434\u044B \u0441 \u0447\u0451\u0440\u043D\u043E\u0439 \u0434\u044B\u0440\u043E\u0439."@ru . . . . . . . . . "Kilonova"@cs . "Kilonova"@pt . . . . . . . "Kilonowa (ang. kilonova) \u2013 zjawisko astronomiczne polegaj\u0105ce na zderzeniu dw\u00F3ch gwiazd zdegenerowanych (np. gwiazd neutronowych) lub gwiazdy neutronowej i czarnej dziury, kt\u00F3re jest najprawdopodobniej odpowiedzialne za bardzo kr\u00F3tkie rozb\u0142yski gamma. W wybuchach typu kilonowa wytwarzane s\u0105 bardzo du\u017Ce ilo\u015Bci ci\u0119\u017Ckich metali w ramach procesu r. Nazwa zjawiska pochodzi od po\u0142\u0105czenia dw\u00F3ch s\u0142\u00F3w kilo (tysi\u0105c) i nowa i oznacza, \u017Ce typowa kilonowa wybucha z moc\u0105 tysi\u0119cy zwyk\u0142ych nowych klasycznych. Pierwszym odkrytym tego typu zjawiskiem jest prawdopodobnie rozb\u0142ysk gamma ."@pl . . . . . . . . "Een kilonova (macronova of r-proces supernova) is een voorbijgaande astronomische gebeurtenis die zich voordoet in een compact binair systeem wanneer twee neutronensterren of een neutronenster en een zwart gat in elkaar opgaan. Kilonovae worden gedacht korte gammaflitsen en sterke elektromagnetische straling uit te zenden door het radioactief verval van zware r-proces kernen die tijdens het fusieproces vrij isotropisch worden geproduceerd en uitgeworpen. De eerste kilonova werd waargenomen in 2013 met behulp van de ruimtetelescoop Hubble."@nl . . "Kilonova"@fr . "Une kilonova, aussi nomm\u00E9e macronova ou supernova \u00E0 processus r, est un ph\u00E9nom\u00E8ne astronomique qui se produit lors de la fusion de deux \u00E9toile \u00E0 neutrons ou d'une \u00E9toile \u00E0 neutron et d'un trou noir, dans un syst\u00E8me binaire. Un rayonnement \u00E9lectromagn\u00E9tique intense est \u00E9mis du fait de la d\u00E9sint\u00E9gration d'ions lourds produits par processus r et \u00E9ject\u00E9s de fa\u00E7on relativement isotrope pendant le processus de fusion \u2014 comme pour une br\u00E8ve supernova de faible luminosit\u00E9. Entre 2017 et 2021, la communaut\u00E9 scientifique a identifi\u00E9 environ 50 signaux qui seraient issus de kilonovae."@fr . "Eine Kilonova (alternativ auch Macronova) ist der Helligkeitsausbruch eines verschmelzenden Doppelsterns, dessen elektromagnetische Strahlung durch den radioaktiven Zerfall von Elementen angetrieben wird, die im r-Prozess gebildet wurden. Der Begriff Kilonova bezieht sich auf die freigesetzte Energie, die ungef\u00E4hr den tausendfachen Wert einer klassischen Nova erreicht und lichtschw\u00E4cher ist als eine normale Supernova."@de . . . "1112151564"^^ . . "\uD0AC\uB85C\uB178\uBC14(kilonova)\uB294 \uC911\uC131\uC790\uBCC4 \uC30D\uC774\uB098 \uC911\uC131\uC790\uBCC4\uACFC \uBE14\uB799\uD640\uB85C \uC774\uB8E8\uC5B4\uC9C4 \uC5F0\uC131\uACC4\uC5D0\uC11C \uB450 \uCC9C\uCCB4\uAC00 \uCDA9\uB3CC\uD560 \uB54C \uC77C\uC5B4\uB098\uB294 \uC21C\uAC04\uC801\uC778 \uD604\uC0C1\uC73C\uB85C, \uB9E4\uD06C\uB85C\uB178\uBC14(macronova)\uB098 R-\uACFC\uC815 \uCD08\uC2E0\uC131(r-process supernova)\uC774\uB77C\uACE0\uB3C4 \uD55C\uB2E4. \uD0AC\uB85C\uB178\uBC14\uB294 \uBB34\uAC70\uC6B4 R-\uACFC\uC815 \uD575\uC774 \uB4F1\uBC29\uC801\uC73C\uB85C \uBC29\uC0AC\uC131 \uBD95\uAD34\uD558\uC5EC \uC9E7\uC740 \uAC10\uB9C8\uC120 \uD3ED\uBC1C\uC744 \uC77C\uC73C\uD0AC \uAC83\uC774\uB77C\uACE0 \uC5EC\uACA8\uC9C4\uB2E4. \uD0AC\uB85C\uB178\uBC14\uB77C\uB294 \uC6A9\uC5B4\uB294 \uD0AC\uB85C\uB178\uBC14\uC758 \uCD5C\uACE0 \uBC1D\uAE30\uAC00 \uC77C\uBC18\uC801\uC778 \uC2E0\uC131(\uB178\uBC14)\uC758 1000\uBC30 \uC815\uB3C4\uB77C\uB294 \uC810\uC5D0\uC11C \uC81C\uC548\uB418\uC5C8\uC73C\uBA70, \uC774\uB294 \uC77C\uBC18\uC801\uC778 \uCD08\uC2E0\uC131 \uBC1D\uAE30\uC758 10~100\uBC30 \uC815\uB3C4\uC774\uB2E4. \uCD5C\uCD08\uB85C \uBC1C\uACAC\uB41C \uD0AC\uB85C\uB178\uBC14\uB294 \uAC10\uB9C8\uC120 \uD3ED\uBC1C SGRB 130603B\uB85C, \uC2A4\uC704\uD504\uD2B8 \uAC10\uB9C8\uC120 \uD3ED\uBC1C \uC784\uBB34, WIND, \uD5C8\uBE14 \uC6B0\uC8FC \uB9DD\uC6D0\uACBD\uC744 \uD1B5\uD574 \uAD00\uCE21\uD558\uC600\uB2E4. 2018\uB144 10\uC6D4, 2015\uB144 \uBC1C\uACAC\uB41C \uAC10\uB9C8\uC120 \uD3ED\uBC1C \uAC00 2017\uB144 \uBC1C\uACAC\uB41C \uC911\uB825\uD30C \uACFC \uC720\uC0AC\uD55C \uD604\uC0C1\uC774\uB77C\uB294 \uC8FC\uC7A5\uC774 \uC81C\uAE30\uB418\uC5C8\uB2E4. \uB2E4\uC591\uD55C \uC804\uC790\uAE30\uD30C\uB85C \uAD00\uCE21\uD55C \uBAA8\uC2B5\uC774\uB098 \uD604\uC0C1\uC774 \uC77C\uC5B4\uB09C \uC740\uD558\uC758 \uD658\uACBD \uB4F1\uC774 \uB9E4\uC6B0 \uC720\uC0AC\uD558\uC5EC \uBCC4\uAC1C\uC758 \uC0AC\uAC74\uCC98\uB7FC \uBCF4\uC774\uB294 \uB450 \uD604\uC0C1\uC774 \uC0AC\uC2E4\uC740 \uC911\uC131\uC790\uBCC4\uC758 \uCDA9\uB3CC\uC774\uB77C\uB294 \uAC19\uC740 \uC6D0\uC778\uC73C\uB85C \uC77C\uC5B4\uB09C \uC0AC\uAC74\uC73C\uB85C, \uB458 \uBAA8\uB450 \uD0AC\uB85C\uB178\uBC14\uC758 \uACFC\uB3C4\uC801\uC778 \uC0C1\uD0DC\uB77C\uB294 \uAC83\uC73C\uB85C, \uC774 \uC8FC\uC7A5\uC774 \uB9DE\uB2E4\uBA74 \uAE30\uC874\uC5D0 \uCD94\uC815\uB418\uC5C8\uB358 \uAC83\uBCF4\uB2E4 \uD0AC\uB85C\uB178\uBC14\uB294 \uC0C1\uB2F9\uD788 \uD754\uD55C \uD604\uC0C1\uC73C\uB85C \uC608\uCE21\uB41C\uB2E4."@ko . . . "10415"^^ . "Una kilonova (tambi\u00E9n llamada macronova o proceso de supernova de tipo r) ocurre cuando dos estrellas de neutrones o una estrella de neutrones y un agujero negro se fusionan a partir de un sistema binario. Por lo general emiten fuertes se\u00F1ales de radiaci\u00F3n electromagn\u00E9tica debido al proceso de desintegraci\u00F3n de iones pesados que son producidos y expulsados de forma isotr\u00F3pica durante el proceso de fusi\u00F3n. Ser\u00EDa muy similar a una supernova, pero m\u00E1s corta y con menor emisi\u00F3n.\u200BUn tiempo antes de la fusi\u00F3n, ambos objetos compactos empiezan a rotar sobre el centro de masas del sistema binario muy r\u00E1pidamente, lo cual se teoriz\u00F3 que podr\u00EDa ser una fuente importante de ondas gravitacionales (GWs).\u200B En octubre de 2017 se pudo demostrar finalmente dicha teor\u00EDa mediante resultados experimentales. E"@es . . . "Kilonova"@de . . . . . . . . "\uD0AC\uB85C\uB178\uBC14"@ko . "\u30AD\u30ED\u30CE\u30F4\u30A1\uFF08\u82F1: kilonova, macronova\uFF09\u306F\u3001\u9AD8\u5BC6\u5EA6\u306E\u5929\u4F53\u304C\u878D\u5408\u3059\u308B\u969B\u306B\u8D77\u3053\u308B\u5927\u898F\u6A21\u306A\u7206\u767A\u73FE\u8C61\u3067\u3042\u308B\u3002\u305D\u306E\u96FB\u78C1\u653E\u5C04\u306F\u3001r\u904E\u7A0B\u306B\u3088\u3063\u3066\u751F\u3058\u305F\u5143\u7D20\u304C\u653E\u5C04\u6027\u5D29\u58CA\u3092\u8D77\u3053\u3059\u3053\u3068\u306B\u3088\u3063\u3066\u751F\u3058\u308B\u3002\u30AD\u30ED\u30CE\u30D0\u3068\u3082\u8868\u8A18\u3055\u308C\u308B\u3002"@ja . "Kilonova"@en . . . . . . . . "Una kilonova \u00E8 una esplosione astronomica che si verifica quando due oggetti celesti superdensi, come stelle di neutroni e buchi neri, si fondono tra loro. La loro luminosit\u00E0 \u00E8 1000 volte pi\u00F9 intensa di quella di una stella nova e da 1/10 a 1/100 di quella di una supernova. Lo spettro energetico di una kilonova \u00E8 concentrato prevalentemente nella zona dell'infrarosso vicino, a causa dell'elevata produzione di elementi radioattivi pesanti e ricchi di neutroni che fungerebbero da \"filtro\" alle radiazioni con frequenze pi\u00F9 elevate. Durante la coalescenza dei due oggetti progenitori fino alla fusione, una kilonova \u00E8 anche una forte sorgente di onde gravitazionali. L'emissione di onde gravitazionali, lampo gamma, raggi X, raggi UV, luce visibile, radiazione infrarossa e onde radio osservata a seguito dell'evento GW170817 sembrerebbe essere associata ad una kilonova risultante dalla fusione di due stelle di neutroni. Ad ottobre 2017, un gruppo di astronomi a guida italiana, utilizzando lo strumento X-shooter del VLT, ha rilevato il primo spettro di una kilonova."@it . . . . "Kilonova je astronomick\u00E1 ud\u00E1lost, p\u0159i n\u00ED\u017E dojde ke splynut\u00ED dvou neutronov\u00FDch hv\u011Bzd nebo neutronov\u00E9 hv\u011Bzdy a \u010Dern\u00E9 d\u00EDry. Tento jev je p\u0159ibli\u017En\u011B 1000\u00D7 jasn\u011Bj\u0161\u00ED ne\u017E b\u011B\u017En\u00E1 nova \u2013 z toho vych\u00E1z\u00ED jej\u00ED n\u00E1zev. Kilonova se pova\u017Euje za jeden z pravd\u011Bpodobn\u00FDch zdroj\u016F gama z\u00E1blesk\u016F a siln\u00E9ho elektromagnetick\u00E9ho z\u00E1\u0159en\u00ED vznikaj\u00EDc\u00EDho v d\u016Fsledku radioaktivn\u00EDho rozpadu nov\u011B vznikl\u00FDch prvk\u016F."@cs . "Une kilonova, aussi nomm\u00E9e macronova ou supernova \u00E0 processus r, est un ph\u00E9nom\u00E8ne astronomique qui se produit lors de la fusion de deux \u00E9toile \u00E0 neutrons ou d'une \u00E9toile \u00E0 neutron et d'un trou noir, dans un syst\u00E8me binaire. Un rayonnement \u00E9lectromagn\u00E9tique intense est \u00E9mis du fait de la d\u00E9sint\u00E9gration d'ions lourds produits par processus r et \u00E9ject\u00E9s de fa\u00E7on relativement isotrope pendant le processus de fusion \u2014 comme pour une br\u00E8ve supernova de faible luminosit\u00E9. Entre 2017 et 2021, la communaut\u00E9 scientifique a identifi\u00E9 environ 50 signaux qui seraient issus de kilonovae."@fr . . . "\u0645\u0633\u062A\u0639\u0631 \u0645\u0627\u0643\u0631\u0648 (\u064A\u0633\u0645\u0649 \u0623\u064A\u0636\u0627 \u0643\u064A\u0644\u0648\u0646\u0648\u0641\u0627 \u00AB\u0645\u0627\u0643\u0631\u0648\u0646\u0648\u0641\u0627\u00BB \u0623\u0648 \u00AB\u0645\u0633\u062A\u0639\u0631 \u0623\u0639\u0638\u0645 \u0639\u0645\u0644\u064A\u0629 \u0627\u0644\u062A\u0642\u0627\u0637 \u0627\u0644\u0646\u064A\u0648\u062A\u0631\u0648\u0646 \u0627\u0644\u0633\u0631\u064A\u0639\u0629\u00BB (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: r-process supernova)\u200F) \u062D\u062F\u062B \u0641\u0644\u0643\u064A \u064A\u062D\u062F\u062B \u0639\u0646\u062F\u0645\u0627 \u064A\u0646\u062F\u0645\u062C \u0646\u062C\u0645\u0627\u0646 \u0646\u064A\u0648\u062A\u0631\u0648\u0646 \u0623\u0648 \u0646\u062C\u0645 \u0646\u064A\u0648\u062A\u0631\u0648\u0646\u064A \u0648\u062B\u0642\u0628 \u0623\u0633\u0648\u062F \u0641\u064A \u0646\u0638\u0627\u0645 \u062B\u0646\u0627\u0626\u064A. \u064A\u0646\u0628\u0639\u062B \u0627\u0644\u0625\u0634\u0639\u0627\u0639 \u0627\u0644\u0643\u0647\u0631\u0648\u0645\u063A\u0646\u0627\u0637\u064A\u0633\u064A \u0627\u0644\u0642\u0648\u064A \u0628\u0633\u0628\u0628 \u0627\u0646\u062D\u0644\u0627\u0644 \u0627\u0644\u0623\u064A\u0648\u0646\u0627\u062A \u0627\u0644\u062B\u0642\u064A\u0644\u0629 \u0645\u0646 \u0639\u0645\u0644\u064A\u0629 \u0627\u0644\u062A\u0642\u0627\u0637 \u0627\u0644\u0646\u064A\u0648\u062A\u0631\u0648\u0646 \u0627\u0644\u0633\u0631\u064A\u0639\u0629 \u0627\u0644\u062A\u064A \u064A\u062A\u0645 \u0625\u0646\u062A\u0627\u062C\u0647\u0627 \u0648\u0625\u062E\u0631\u0627\u062C\u0647\u0627 \u0625\u0644\u0649 \u062D\u062F \u0645\u0627 \u062E\u0644\u0627\u0644 \u0639\u0645\u0644\u064A\u0629 \u0625\u0646\u062F\u0645\u0627\u062C \u0627\u0644\u062E\u0648\u0627\u0635 - \u0639\u0644\u0649 \u063A\u0631\u0627\u0631 \u0645\u0633\u062A\u0639\u0631 \u0623\u0639\u0638\u0645 \u0642\u0635\u064A\u0631 \u0627\u0644\u0623\u062C\u0644 \u062E\u0627\u0641\u062A.\u0648\u064A\u0639\u062A\u0642\u062F \u0623\u0646 \u0639\u0645\u0644\u064A\u0629 \u0627\u0646\u062F\u0645\u0627\u062C \u0648\u0645\u0633\u0627\u0631 \u0647\u0630\u0627 \u0627\u0644\u0632\u0648\u062C \u0645\u0646 \u0627\u0644\u0646\u062C\u0648\u0645 \u0627\u0644\u062B\u0646\u0627\u0626\u064A\u0629 \u0645\u0635\u062F\u0631 \u0645\u0648\u062C\u0627\u062A \u062C\u0627\u0630\u0628\u064A\u0629 \u0642\u0648\u064A."@ar . . . . . "Kilonova"@ca . . . . "\u5343\u65B0\u661F"@zh . . "40167806"^^ . . "Una kilonova (tamb\u00E9 coneguda com a macronova o supernova de proc\u00E9s R) \u00E9s un esdeveniment transitori astron\u00F2mic que succeeix quan es fusionen dues estrelles de neutrons o una estrella de neutrons i un forat negre. S'ha teoritzat que aquest esdeveniment emet un esclat de raigs gamma i altra radiaci\u00F3 electromagn\u00E8tica pel deca\u00EFment de nuclis pesants pel proc\u00E9s radioactiu R que es produeixen i s'ejecten de forma isot\u00F2pica durant el proc\u00E9s de fusi\u00F3. La primera kilonova va ser detectada el 2013 pel telescopi espacial Hubble associada a l'esclat de raigs gamma GRB 130603B."@ca . "Kilonova"@in . . . . "Kilonowa"@pl . . "\u0645\u0633\u062A\u0639\u0631 \u0645\u0627\u0643\u0631\u0648 (\u064A\u0633\u0645\u0649 \u0623\u064A\u0636\u0627 \u0643\u064A\u0644\u0648\u0646\u0648\u0641\u0627 \u00AB\u0645\u0627\u0643\u0631\u0648\u0646\u0648\u0641\u0627\u00BB \u0623\u0648 \u00AB\u0645\u0633\u062A\u0639\u0631 \u0623\u0639\u0638\u0645 \u0639\u0645\u0644\u064A\u0629 \u0627\u0644\u062A\u0642\u0627\u0637 \u0627\u0644\u0646\u064A\u0648\u062A\u0631\u0648\u0646 \u0627\u0644\u0633\u0631\u064A\u0639\u0629\u00BB (\u0628\u0627\u0644\u0625\u0646\u062C\u0644\u064A\u0632\u064A\u0629: r-process supernova)\u200F) \u062D\u062F\u062B \u0641\u0644\u0643\u064A \u064A\u062D\u062F\u062B \u0639\u0646\u062F\u0645\u0627 \u064A\u0646\u062F\u0645\u062C \u0646\u062C\u0645\u0627\u0646 \u0646\u064A\u0648\u062A\u0631\u0648\u0646 \u0623\u0648 \u0646\u062C\u0645 \u0646\u064A\u0648\u062A\u0631\u0648\u0646\u064A \u0648\u062B\u0642\u0628 \u0623\u0633\u0648\u062F \u0641\u064A \u0646\u0638\u0627\u0645 \u062B\u0646\u0627\u0626\u064A. \u064A\u0646\u0628\u0639\u062B \u0627\u0644\u0625\u0634\u0639\u0627\u0639 \u0627\u0644\u0643\u0647\u0631\u0648\u0645\u063A\u0646\u0627\u0637\u064A\u0633\u064A \u0627\u0644\u0642\u0648\u064A \u0628\u0633\u0628\u0628 \u0627\u0646\u062D\u0644\u0627\u0644 \u0627\u0644\u0623\u064A\u0648\u0646\u0627\u062A \u0627\u0644\u062B\u0642\u064A\u0644\u0629 \u0645\u0646 \u0639\u0645\u0644\u064A\u0629 \u0627\u0644\u062A\u0642\u0627\u0637 \u0627\u0644\u0646\u064A\u0648\u062A\u0631\u0648\u0646 \u0627\u0644\u0633\u0631\u064A\u0639\u0629 \u0627\u0644\u062A\u064A \u064A\u062A\u0645 \u0625\u0646\u062A\u0627\u062C\u0647\u0627 \u0648\u0625\u062E\u0631\u0627\u062C\u0647\u0627 \u0625\u0644\u0649 \u062D\u062F \u0645\u0627 \u062E\u0644\u0627\u0644 \u0639\u0645\u0644\u064A\u0629 \u0625\u0646\u062F\u0645\u0627\u062C \u0627\u0644\u062E\u0648\u0627\u0635 - \u0639\u0644\u0649 \u063A\u0631\u0627\u0631 \u0645\u0633\u062A\u0639\u0631 \u0623\u0639\u0638\u0645 \u0642\u0635\u064A\u0631 \u0627\u0644\u0623\u062C\u0644 \u062E\u0627\u0641\u062A.\u0648\u064A\u0639\u062A\u0642\u062F \u0623\u0646 \u0639\u0645\u0644\u064A\u0629 \u0627\u0646\u062F\u0645\u0627\u062C \u0648\u0645\u0633\u0627\u0631 \u0647\u0630\u0627 \u0627\u0644\u0632\u0648\u062C \u0645\u0646 \u0627\u0644\u0646\u062C\u0648\u0645 \u0627\u0644\u062B\u0646\u0627\u0626\u064A\u0629 \u0645\u0635\u062F\u0631 \u0645\u0648\u062C\u0627\u062A \u062C\u0627\u0630\u0628\u064A\u0629 \u0642\u0648\u064A."@ar . "Eine Kilonova (alternativ auch Macronova) ist der Helligkeitsausbruch eines verschmelzenden Doppelsterns, dessen elektromagnetische Strahlung durch den radioaktiven Zerfall von Elementen angetrieben wird, die im r-Prozess gebildet wurden. Der Begriff Kilonova bezieht sich auf die freigesetzte Energie, die ungef\u00E4hr den tausendfachen Wert einer klassischen Nova erreicht und lichtschw\u00E4cher ist als eine normale Supernova."@de . . "\u041A\u0438\u043B\u043E\u043D\u043E\u0432\u0430\u044F"@ru . . "\u30AD\u30ED\u30CE\u30F4\u30A1\uFF08\u82F1: kilonova, macronova\uFF09\u306F\u3001\u9AD8\u5BC6\u5EA6\u306E\u5929\u4F53\u304C\u878D\u5408\u3059\u308B\u969B\u306B\u8D77\u3053\u308B\u5927\u898F\u6A21\u306A\u7206\u767A\u73FE\u8C61\u3067\u3042\u308B\u3002\u305D\u306E\u96FB\u78C1\u653E\u5C04\u306F\u3001r\u904E\u7A0B\u306B\u3088\u3063\u3066\u751F\u3058\u305F\u5143\u7D20\u304C\u653E\u5C04\u6027\u5D29\u58CA\u3092\u8D77\u3053\u3059\u3053\u3068\u306B\u3088\u3063\u3066\u751F\u3058\u308B\u3002\u30AD\u30ED\u30CE\u30D0\u3068\u3082\u8868\u8A18\u3055\u308C\u308B\u3002"@ja . . . . "\u041A\u0438\u043B\u043E\u043D\u00F3\u0432\u0430\u044F (kilonova) \u2014 \u044D\u0442\u043E \u0430\u0441\u0442\u0440\u043E\u043D\u043E\u043C\u0438\u0447\u0435\u0441\u043A\u043E\u0435 \u0441\u043E\u0431\u044B\u0442\u0438\u0435, \u043F\u0440\u043E\u0438\u0441\u0445\u043E\u0434\u044F\u0449\u0435\u0435 \u0432 \u0434\u0432\u043E\u0439\u043D\u044B\u0445 \u0437\u0432\u0451\u0437\u0434\u043D\u044B\u0445 \u0441\u0438\u0441\u0442\u0435\u043C\u0430\u0445 \u043F\u0440\u0438 \u0441\u043B\u0438\u044F\u043D\u0438\u0438 \u0434\u0432\u0443\u0445 \u043D\u0435\u0439\u0442\u0440\u043E\u043D\u043D\u044B\u0445 \u0437\u0432\u0451\u0437\u0434 \u0438\u043B\u0438 \u043D\u0435\u0439\u0442\u0440\u043E\u043D\u043D\u043E\u0439 \u0437\u0432\u0435\u0437\u0434\u044B \u0441 \u0447\u0451\u0440\u043D\u043E\u0439 \u0434\u044B\u0440\u043E\u0439."@ru . . . . . "Uma kilonova (tamb\u00E9m chamada de uma 'macronova' ou uma 'supernova de processo-r\") ocorre quando duas estrelas de n\u00EAutrons ou uma estrela de n\u00EAutron e um buraco negro se unem em um sistema bin\u00E1rio. Uma forte radia\u00E7\u00E3o eletromagn\u00E9tica \u00E9 emitida devido ao decaimento de \u00EDons do pesado processo-r que s\u00E3o produzidos e ejetados basicamente na forma isotr\u00F3pica durante o processo de fus\u00E3o \u2014 semelhante a uma supernova fraca e de curta dura\u00E7\u00E3o.O espiral e a fus\u00E3o dos dois objetos compactos s\u00E3o uma forte fonte de ondas gravitacionais (GWs). Acredita-se que possa ser o emissor de curtas explos\u00F5es de raios gama e a fonte predominante do est\u00E1vel processo-r de elementos no Universo."@pt . "Una kilonova (tamb\u00E9 coneguda com a macronova o supernova de proc\u00E9s R) \u00E9s un esdeveniment transitori astron\u00F2mic que succeeix quan es fusionen dues estrelles de neutrons o una estrella de neutrons i un forat negre. S'ha teoritzat que aquest esdeveniment emet un esclat de raigs gamma i altra radiaci\u00F3 electromagn\u00E8tica pel deca\u00EFment de nuclis pesants pel proc\u00E9s radioactiu R que es produeixen i s'ejecten de forma isot\u00F2pica durant el proc\u00E9s de fusi\u00F3. La primera kilonova va ser detectada el 2013 pel telescopi espacial Hubble associada a l'esclat de raigs gamma GRB 130603B."@ca . . "Kilonowa (ang. kilonova) \u2013 zjawisko astronomiczne polegaj\u0105ce na zderzeniu dw\u00F3ch gwiazd zdegenerowanych (np. gwiazd neutronowych) lub gwiazdy neutronowej i czarnej dziury, kt\u00F3re jest najprawdopodobniej odpowiedzialne za bardzo kr\u00F3tkie rozb\u0142yski gamma. W wybuchach typu kilonowa wytwarzane s\u0105 bardzo du\u017Ce ilo\u015Bci ci\u0119\u017Ckich metali w ramach procesu r. Nazwa zjawiska pochodzi od po\u0142\u0105czenia dw\u00F3ch s\u0142\u00F3w kilo (tysi\u0105c) i nowa i oznacza, \u017Ce typowa kilonowa wybucha z moc\u0105 tysi\u0119cy zwyk\u0142ych nowych klasycznych. Zderzenia tego typu obiekt\u00F3w by\u0142y badane mi\u0119dzy innymi przez polskiego astronoma Bohdana Paczy\u0144skiego, kt\u00F3ry wraz z opracowa\u0142 pierwsze teoretyczne modele takich zderze\u0144. Pierwszym odkrytym tego typu zjawiskiem jest prawdopodobnie rozb\u0142ysk gamma . 12 marca 2018 ponad 30 radioteleskop\u00F3w zbada\u0142o kilonow\u0105 , powsta\u0142\u0105 w wyniku po\u0142\u0105czenia dw\u00F3ch gwiazd neutronowych w galaktyce NGC 4993. Zjawisku towarzyszy\u0142a emisja fal grawitacyjnych (sygna\u0142 ), zarejestrowana 17 sierpnia 2017 roku."@pl . . . .