About: GS 2000+25

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http://dbpedia.org/describe/?url=http%3A%2F%2Fdbpedia.org%2Fresource%2FGS_2000%2B25

GS 2000+25 is an X-ray binary system in the constellation Vulpecula, consisting of a late K-type star and a black hole. It is also an X-ray nova.

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body star
rdfs:label	GS 2000+25 (en) GS2000+25 (it) GS 2000+25 (sv)
rdfs:comment	GS 2000+25 is an X-ray binary system in the constellation Vulpecula, consisting of a late K-type star and a black hole. It is also an X-ray nova. (en) GS2000+25 è un sistema binario a raggi X formato da un buco nero ed una stella di classe K di magnitudine 18,2. La componente secondaria del sistema, una nana arancione, ruota attorno ad un oggetto compatto di massa 8,5 ± 1,5 masse solari in 0,344098 giorni. GS2000+25 fu scoperta come nova a raggi X il 26 aprile 1988 dal satellite Ginga durante un'esplosione derivata dalla caduta di materia del disco di accrescimento sul buco nero . (it) GS 2000+25, även känd som Nova Vulpeculae 1988 och QZ Vulpeculae, är en dubbelstjärna i den mellersta delen av stjärnbilden Räven upptäckt år 1988 (Tsunemi et al. 1989). Den består av en sen stjärna av spektralklass K3-6 V och ett svart hål. (sv)
foaf:depiction
dcterms:subject	K-type main-sequence stars Objects with variable star designations Vulpecula Stellar black holes Novae
Wikipage page ID	54136404 (xsd:integer)
Wikipage revision ID	1118974542 (xsd:integer)
Link from a Wikipage to another Wikipage	Black hole List of nearest black holes Light curve K-type main-sequence stars Objects with variable star designations Vulpecula Constellation X-ray binary Vulpecula Stellar black holes J2000 Novae K-type star Solar mass Photometric system X-ray nova
sameAs	GS 2000+25 GS 2000+25 GS 2000+25 GS 2000+25
dbp:wikiPageUsesTemplate	dbt:More_citations_needed dbt:Reflist dbt:Short_description dbt:Starbox_astrometry dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_character dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_image dbt:Starbox_observe dbt:Starbox_orbit dbt:Starbox_reference dbt:Stars_of_Vulpecula dbt:Var-star-stub dbt:DEC dbt:Odlist dbt:RA dbt:Multi-star-stub
thumbnail	wiki-commons:Special:FilePath/QZVulLightCurve.png?width=300
dist ly	8800 (xsd:integer)
appmag v	18.200000 (xsd:double)
component	Black hole (en)
constell	Vulpecula
dist pc	2700 (xsd:integer)
epoch	J2000
mass	7.200000 (xsd:double)
has abstract	GS 2000+25 is an X-ray binary system in the constellation Vulpecula, consisting of a late K-type star and a black hole. It is also an X-ray nova. (en) GS2000+25 è un sistema binario a raggi X formato da un buco nero ed una stella di classe K di magnitudine 18,2. La componente secondaria del sistema, una nana arancione, ruota attorno ad un oggetto compatto di massa 8,5 ± 1,5 masse solari in 0,344098 giorni. GS2000+25 fu scoperta come nova a raggi X il 26 aprile 1988 dal satellite Ginga durante un'esplosione derivata dalla caduta di materia del disco di accrescimento sul buco nero . (it) GS 2000+25, även känd som Nova Vulpeculae 1988 och QZ Vulpeculae, är en dubbelstjärna i den mellersta delen av stjärnbilden Räven upptäckt år 1988 (Tsunemi et al. 1989). Den består av en sen stjärna av spektralklass K3-6 V och ett svart hål. Eftersom det svarta hålet är mer massivt än följeslagaren, är detta den primära komponenten i konstellationen. Det svarta hålet bedöms ha en massa som är ca 5 gånger större än solens medan följeslagaren har en massa av ca 0,5 solmassor. Eftersom den följeslagande stjärnan har en liten massa är stjärnparet en röntgenstrålande dubbelstjärna med låg massa. Stjärnorna cirkulerar kring varandra med en omloppsperiod av 8,26 timmar. (sv)
prov:wasDerivedFrom	wikipedia-en:GS_2000+25?oldid=1118974542&ns=0
page length (characters) of wiki page	3966 (xsd:nonNegativeInteger)
foaf:isPrimaryTopicOf	wikipedia-en:GS_2000+25
is Link from a Wikipage to another Wikipage of	List of black holes List of nearest known black holes Stellar black hole List of stars in Vulpecula QZ Vulpeculae
is Wikipage redirect of	QZ Vulpeculae
is foaf:primaryTopic of	wikipedia-en:GS_2000+25

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