About: GRB 101225A     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:YagoPermanentlyLocatedEntity, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)
QRcode icon
http://dbpedia.demo.openlinksw.com/describe/?url=http%3A%2F%2Fdbpedia.org%2Fresource%2FGRB_101225A&invfp=IFP_OFF&sas=SAME_AS_OFF

GRB 101225A, also known as the "Christmas burst", was a cosmic explosion first detected by NASA's Swift observatory on Christmas Day 2010. The gamma-ray emission lasted at least 28 minutes, which is unusually long. Follow-up observations of the burst's afterglow by the Hubble Space Telescope and ground-based observatories were unable to determine the object's distance using spectroscopic methods.

AttributesValues
rdf:type
rdfs:label
  • GRB 101225A (en)
  • GRB 101225A (ja)
  • GRB 101225A (pl)
rdfs:comment
  • GRB 101225Aとは、2010年12月25日にアンドロメダ座の方向に発生したガンマ線バーストである。ガンマ線放出の継続時間が約28分と非常に長いことが特徴である。発生日時から通称「クリスマスバースト (Christmas burst)」とも呼ばれる。GRB 101225Aの発見は、ガンマ線バーストの種類がより多様であることを示している。 (ja)
  • GRB 101225A (tzw. „rozbłysk bożonarodzeniowy”) – nietypowy rozbłysk gamma wykryty przez satelitę Swift 25 grudnia 2010 roku w gwiazdozbiorze Andromedy. Rozbłysk był nietypowy z dwóch powodów. Po pierwsze był jednym z najdłuższych rozbłysków (28 minut), a po drugie nie jest dotychczas znana odległość do jego źródła ani też natura tego rozbłysku. (pl)
  • GRB 101225A, also known as the "Christmas burst", was a cosmic explosion first detected by NASA's Swift observatory on Christmas Day 2010. The gamma-ray emission lasted at least 28 minutes, which is unusually long. Follow-up observations of the burst's afterglow by the Hubble Space Telescope and ground-based observatories were unable to determine the object's distance using spectroscopic methods. (en)
dcterms:subject
Wikipage page ID
Wikipage revision ID
Link from a Wikipage to another Wikipage
Link from a Wikipage to an external page
sameAs
dbp:wikiPageUsesTemplate
has abstract
  • GRB 101225A, also known as the "Christmas burst", was a cosmic explosion first detected by NASA's Swift observatory on Christmas Day 2010. The gamma-ray emission lasted at least 28 minutes, which is unusually long. Follow-up observations of the burst's afterglow by the Hubble Space Telescope and ground-based observatories were unable to determine the object's distance using spectroscopic methods. In papers published in the journal Nature, two different groups of astronomers proposed different theories about the event's origin. Sergio Campana's group proposes that the event was caused by a comet crashing onto a neutron star within our own galaxy. Christina Thöne's group prefers a more conventional supernova mechanism, involving a merger between a helium star and a neutron star at a distance of about 5.5 billion light years from Earth. (en)
  • GRB 101225Aとは、2010年12月25日にアンドロメダ座の方向に発生したガンマ線バーストである。ガンマ線放出の継続時間が約28分と非常に長いことが特徴である。発生日時から通称「クリスマスバースト (Christmas burst)」とも呼ばれる。GRB 101225Aの発見は、ガンマ線バーストの種類がより多様であることを示している。 (ja)
  • GRB 101225A (tzw. „rozbłysk bożonarodzeniowy”) – nietypowy rozbłysk gamma wykryty przez satelitę Swift 25 grudnia 2010 roku w gwiazdozbiorze Andromedy. Rozbłysk był nietypowy z dwóch powodów. Po pierwsze był jednym z najdłuższych rozbłysków (28 minut), a po drugie nie jest dotychczas znana odległość do jego źródła ani też natura tego rozbłysku. (pl)
gold:hypernym
prov:wasDerivedFrom
page length (characters) of wiki page
foaf:isPrimaryTopicOf
is Link from a Wikipage to another Wikipage of
is Wikipage redirect of
is foaf:primaryTopic of
Faceted Search & Find service v1.17_git139 as of Feb 29 2024


Alternative Linked Data Documents: ODE     Content Formats:   [cxml] [csv]     RDF   [text] [turtle] [ld+json] [rdf+json] [rdf+xml]     ODATA   [atom+xml] [odata+json]     Microdata   [microdata+json] [html]    About   
This material is Open Knowledge   W3C Semantic Web Technology [RDF Data] Valid XHTML + RDFa
OpenLink Virtuoso version 08.03.3330 as of Mar 19 2024, on Linux (x86_64-generic-linux-glibc212), Single-Server Edition (378 GB total memory, 52 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software