About: V598 Puppis     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:Whole100003553, within Data Space : dbpedia.org associated with source document(s)
QRcode icon
http://dbpedia.org/describe/?url=http%3A%2F%2Fdbpedia.org%2Fresource%2FV598_Puppis&graph=http%3A%2F%2Fdbpedia.org&graph=http%3A%2F%2Fdbpedia.org

V598 Puppis is the name given to a nova in the Milky Way Galaxy. USNO-A2.0 0450-03360039, the catalog number for the star, was discovered to be much brighter than normal in X-ray emissions on October 9, 2007, by the European Space Agency's XMM-Newton telescope. Ultimately, the star was confirmed to 600 times brighter than normal by the Magellan-Clay telescope Magellan-Clay telescope at Las Campanas Observatory in Chile. The orbital period of the two stars in V598 Puppis is 0.1628714 days, or 3 hours, 54 minutes, and 32 seconds.

AttributesValues
rdf:type
rdfs:label
  • V598 Puppis (pt)
  • V598 Puppis (en)
rdfs:comment
  • V598 Puppis is the name given to a nova in the Milky Way Galaxy. USNO-A2.0 0450-03360039, the catalog number for the star, was discovered to be much brighter than normal in X-ray emissions on October 9, 2007, by the European Space Agency's XMM-Newton telescope. Ultimately, the star was confirmed to 600 times brighter than normal by the Magellan-Clay telescope Magellan-Clay telescope at Las Campanas Observatory in Chile. The orbital period of the two stars in V598 Puppis is 0.1628714 days, or 3 hours, 54 minutes, and 32 seconds. (en)
  • V598 Puppis é uma nova na galáxia Via Láctea. A estrela foi catalogada como USNO-A2.0 0450-03360039, foi descoberta em 9 de outubro de 2007 por emitir mais raio-X que o normal, pelo telescópio XMM-Newton, da Agência Espacial Europeia. Recentemente foi confirmado que a estrela emite 600 vezes mais raio-X que o normal. Essa confirmação foi feita pelo telescópio Magellan-Clay, no Observatório Las Campanas, no Chile. (pt)
foaf:name
  • V598 Puppis (en)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/V598PupLightCurve.png
dcterms:subject
Wikipage page ID
Wikipage revision ID
Link from a Wikipage to another Wikipage
sameAs
dbp:wikiPageUsesTemplate
thumbnail
appmag v
constell
epoch
  • J2000.0 (en)
prop mo dec
  • −2.3 (en)
prop mo ra
  • −1.0 (en)
radial v
  • +292 (en)
variable
has abstract
  • V598 Puppis is the name given to a nova in the Milky Way Galaxy. USNO-A2.0 0450-03360039, the catalog number for the star, was discovered to be much brighter than normal in X-ray emissions on October 9, 2007, by the European Space Agency's XMM-Newton telescope. Ultimately, the star was confirmed to 600 times brighter than normal by the Magellan-Clay telescope Magellan-Clay telescope at Las Campanas Observatory in Chile. The nova has been officially named V598 Puppis and is "one of the brightest for almost a decade". Despite its brightness, the nova was apparently missed by amateur and professional astronomers alike until XMM-Newton spotted the unusual X-ray source while turning from one target to another. The All Sky Automated Survey determined that that nova had occurred on June 5, 2007. The orbital period of the two stars in V598 Puppis is 0.1628714 days, or 3 hours, 54 minutes, and 32 seconds. (en)
  • V598 Puppis é uma nova na galáxia Via Láctea. A estrela foi catalogada como USNO-A2.0 0450-03360039, foi descoberta em 9 de outubro de 2007 por emitir mais raio-X que o normal, pelo telescópio XMM-Newton, da Agência Espacial Europeia. Recentemente foi confirmado que a estrela emite 600 vezes mais raio-X que o normal. Essa confirmação foi feita pelo telescópio Magellan-Clay, no Observatório Las Campanas, no Chile. A nova foi oficialmente nomeada de V598 Puppis e é "uma das mais brilhantes de quase uma década". Apesar de seu brilho, a nova estava aparentemente perdida por astrônomos amadores e profissionais até que o telescópio XMM-Newton avistou uma fonte incomum de raio-X que gira de um ponto para outro. (pt)
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 08.03.3331 as of Sep 2 2024, on Linux (x86_64-generic-linux-glibc212), Single-Server Edition (62 GB total memory, 39 GB memory in use)
Data on this page belongs to its respective rights holders.
Virtuoso Faceted Browser Copyright © 2009-2024 OpenLink Software