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About: WR 22     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:WikicatEclipsingBinaries, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)

Type: Thingplacedbo:Locationschema:Placecelestial bodyyago:WikicatBinaryStarsyago:WikicatVariableStarsyago:WikicatWolf–RayetStarsyago:WikicatO-typeGiantsyago:WikicatObjectsNamedWithVariableStarDesignationsyago:WikicatStarsyago:Animal100015388yago:BinaryStar109221070yago:CelestialBody109239740yago:Giant101323781yago:LivingThing100004258yago:NaturalObject100019128yago:Object100002684yago:Organism100004475yago:PhysicalEntity100001930yago:WikicatHRObjectsyago:WikicatHenryDraperCatalogueObjectsstaryago:Star109444100yago:VariableStar109469152yago:Whole100003553yago:WikicatEclipsingBinaries New Facet based on Instances of this Class

WR 22, also known as V429 Carinae or HR 4188, is an eclipsing binary star system in the constellation Carina. The system contains a Wolf-Rayet (WR) star that is one of the most massive and most luminous stars known, and is also a bright X-ray source due to colliding winds with a less massive O class companion. Its eclipsing nature and apparent magnitude make it very useful for constraining the properties of luminous hydrogen-rich WR stars.