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Statements

Subject Item
dbr:GR_Muscae
rdf:type
yago:Object100002684 yago:NeutronStar109369692 yago:NaturalObject100019128 yago:WikicatObjectsNamedWithVariableStarDesignations yago:Whole100003553 yago:Star109444100 yago:PhysicalEntity100001930 yago:CelestialBody109239740 yago:BinaryStar109221070 yago:WikicatNeutronStars yago:WikicatX-rayBinaries
rdfs:label
GR Muscae 2S 1254-690
rdfs:comment
GR Muscae, also known as 2S 1254-690 is a binary star system in the constellation Musca composed of a neutron star of between 1.2 and 1.8 times the mass of the Sun and a low-mass star likely to be around the mass of the Sun in close orbit. A magnitude 19 blue star was pinpointed as the optical counterpart of the X-ray source in 1978. Its apparent magnitude varies from 18 to 19.1 over a period of 0.16 days. The neutron star has an accretion disk that takes around 6.74 days to complete a revolution, and is inclined at an angle to the incoming stream of material from the donor star.
dbp:name
GR Muscae
foaf:depiction
n4:GRMusLightCurve.png
dcterms:subject
dbc:Musca_(constellation) dbc:Objects_with_variable_star_designations dbc:Neutron_stars dbc:X-ray_binaries
dbo:wikiPageID
42149345
dbo:wikiPageRevisionID
1068973544
dbo:wikiPageWikiLink
dbr:Neutron_star dbr:Sun n16:GRMusLightCurve.png dbr:Musca_(constellation) dbr:Constellation dbc:Objects_with_variable_star_designations dbc:X-ray_binaries dbc:Neutron_stars dbc:Musca_(constellation)
owl:sameAs
yago-res:GR_Muscae n15:fVM6 freebase:m.0_yf41_ dbpedia-sv:2S_1254-690 wikidata:Q17018608
dbp:wikiPageUsesTemplate
dbt:Reflist dbt:RA dbt:DEC dbt:Starbox_short dbt:Short_description dbt:Var-star-stub dbt:Musca
dbo:thumbnail
n4:GRMusLightCurve.png?width=300
dbp:constell
dbr:Musca_(constellation)
dbo:abstract
GR Muscae, also known as 2S 1254-690 is a binary star system in the constellation Musca composed of a neutron star of between 1.2 and 1.8 times the mass of the Sun and a low-mass star likely to be around the mass of the Sun in close orbit. A magnitude 19 blue star was pinpointed as the optical counterpart of the X-ray source in 1978. Its apparent magnitude varies from 18 to 19.1 over a period of 0.16 days. The neutron star has an accretion disk that takes around 6.74 days to complete a revolution, and is inclined at an angle to the incoming stream of material from the donor star.
gold:hypernym
dbr:System
prov:wasDerivedFrom
wikipedia-en:GR_Muscae?oldid=1068973544&ns=0
dbo:wikiPageLength
2703
foaf:isPrimaryTopicOf
wikipedia-en:GR_Muscae