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Carina OB1 is a giant OB association in the Carina Nebula, which is home to some of the most massive and luminous stars in the Milky Way Galaxy. It includes the young star clusters Collinder 228, NGC 3293, NGC 3324, , Trumpler 14, Trumpler 15 and Trumpler 16, the last being the home of Eta Carinae. It also includes another massive and luminous star, HD 93129A. It is approximately 2,680 parsecs (8,700 ly) from Earth.

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rdf:type
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  • القاعدة OB1 (ar)
  • Carina OB1 (en)
  • Arco della Carena (it)
  • 船底座OB1 (zh)
rdfs:comment
  • القاعدة OB1 هو تجمع نجمي ضخم من النجوم المترابطة ذات التصنيف OB في كوكبة القاعدة داخل حدود سديم القاعدة القاعدة OB1 موطن لبعض النجوم الأكثر سطوعاً في مجرة درب التبانة ويعتبر من مضمن أكبر النجوم المترابطة المعروفة في درب التبانة وأكبر تجمع نجمي للنجوم المترابطة في سديم القاعدة. يشمل تجمع القاعدة OB1 العناقيد النجمية الحديثة النشأة نسبيا ، NGC 3293, NGC 3324, IC 2581, Trumpler 14, Trumpler 15 وTrumpler 16, ويشمل التجمع أيضا نجم ضخم ومضيء آخر . يقع تجمع نجوم القاعدة OB1 بالقرب من نجم إيتا القاعدة على بعد يقدر بنحو 10,000 سنة ضوئية من الأرض. (ar)
  • 船底座OB1是在船底座星雲內的一個巨大OB星協，這是銀河系中一些最巨大和最明亮恆星的家。它包括一些年輕的星團、NGC 3293、NGC 3324、、川普勒14、川普勒15和川普勒16，以及海山二（船底座η）；它也包括另一顆大質量和明亮的恆星HD 93129A。它與地球的距離大約是8,000光年（2,500秒差距）。 它是已知最大的星協之一，其它的還有和天鵝座OB2。因為船底座OB1相對於其他的地區塵埃較少，所以消光也較少。若與船底座OB2結合在一起，它們將會是銀河系中已知規模最大的星協。 船底座OB1的跨距大約70光年（21秒差距），因為位於一個活躍的發射星雲中，是銀河系中最大的星協。它包含許多具有共同特徵的高溫、高光度的恆星。 (zh)
  • Carina OB1 is a giant OB association in the Carina Nebula, which is home to some of the most massive and luminous stars in the Milky Way Galaxy. It includes the young star clusters Collinder 228, NGC 3293, NGC 3324, , Trumpler 14, Trumpler 15 and Trumpler 16, the last being the home of Eta Carinae. It also includes another massive and luminous star, HD 93129A. It is approximately 2,680 parsecs (8,700 ly) from Earth. (en)
  • L'Arco della Carena è una regione della Via Lattea particolarmente ricca di nubi molecolari giganti e di giovanissime ed estese associazioni OB; prende il nome dalla costellazione in cui ricade quasi per intero, quella della Carena. (it)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/NGC_3372d.jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Carina_(Chandra).jpg
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  • القاعدة OB1 هو تجمع نجمي ضخم من النجوم المترابطة ذات التصنيف OB في كوكبة القاعدة داخل حدود سديم القاعدة القاعدة OB1 موطن لبعض النجوم الأكثر سطوعاً في مجرة درب التبانة ويعتبر من مضمن أكبر النجوم المترابطة المعروفة في درب التبانة وأكبر تجمع نجمي للنجوم المترابطة في سديم القاعدة. يشمل تجمع القاعدة OB1 العناقيد النجمية الحديثة النشأة نسبيا ، NGC 3293, NGC 3324, IC 2581, Trumpler 14, Trumpler 15 وTrumpler 16, ويشمل التجمع أيضا نجم ضخم ومضيء آخر . يقع تجمع نجوم القاعدة OB1 بالقرب من نجم إيتا القاعدة على بعد يقدر بنحو 10,000 سنة ضوئية من الأرض. (ar)
  • Carina OB1 is a giant OB association in the Carina Nebula, which is home to some of the most massive and luminous stars in the Milky Way Galaxy. It includes the young star clusters Collinder 228, NGC 3293, NGC 3324, , Trumpler 14, Trumpler 15 and Trumpler 16, the last being the home of Eta Carinae. It also includes another massive and luminous star, HD 93129A. It is approximately 2,680 parsecs (8,700 ly) from Earth. It is one of the largest known stellar associations, along with and Cygnus OB2. It is much easier to see than that of the other associations since Carina OB1 has relatively little dust extinction in its region. Together with Carina OB2, they compromise the most massive stellar grouping known in the galaxy. Carina OB1 is about 70 light-years (21 pc) across, and is the most massive stellar association in the Milky Way Galaxy since it lies within an active emission nebula. It contains many hot luminous stars which share common characteristics. (en)
  • L'Arco della Carena è una regione della Via Lattea particolarmente ricca di nubi molecolari giganti e di giovanissime ed estese associazioni OB; prende il nome dalla costellazione in cui ricade quasi per intero, quella della Carena. È uno dei tratti della Via Lattea tra i più luminosi e congestionati visibili dalla Terra, anche a causa dell'orientamento del braccio di spirale di cui fa parte, il Braccio del Sagittario; questa regione galattica costituisce una delle strutture celesti più caratteristiche visibili dall'emisfero australe ed è dominata in senso assoluto dalla grande e luminosa Nebulosa della Carena, perfettamente visibile anche ad occhio nudo, al cui interno sono attivi importanti processi di formazione stellare, specialmente nei settori più meridionali. A questa si aggiunge un gran numero di nebulose minori, fino a comprendere la cosiddetta "Nebulosa di Lambda Centauri", visibile sul lato più orientale della regione. A riprova della grande attività di formazione stellare, sull'Arco della Carena e nei suoi dintorni sono visibili ben quattro associazioni OB di notevole rilevanza, più un gran numero di ammassi aperti di recente formazione, stelle di Wolf-Rayet e diverse popolazioni di stelle T Tauri. Il vento stellare delle stelle più massicce ha inoltre creato una serie di enormi bolle di vento stellare, i cui bordi sono delimitati da lunghi filamenti di idrogeno neutro e ionizzato. (it)
  • 船底座OB1是在船底座星雲內的一個巨大OB星協，這是銀河系中一些最巨大和最明亮恆星的家。它包括一些年輕的星團、NGC 3293、NGC 3324、、川普勒14、川普勒15和川普勒16，以及海山二（船底座η）；它也包括另一顆大質量和明亮的恆星HD 93129A。它與地球的距離大約是8,000光年（2,500秒差距）。 它是已知最大的星協之一，其它的還有和天鵝座OB2。因為船底座OB1相對於其他的地區塵埃較少，所以消光也較少。若與船底座OB2結合在一起，它們將會是銀河系中已知規模最大的星協。 船底座OB1的跨距大約70光年（21秒差距），因為位於一個活躍的發射星雲中，是銀河系中最大的星協。它包含許多具有共同特徵的高溫、高光度的恆星。 (zh)
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