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H Centauri (H Cen), also known as V945 Centauri, is probable triple star system located in the constellation Centaurus. From parallax measurements, it is located 113 parsecs (370 light years) from the sun. It is a member of the Lower Centaurus–Crux (LCC) subgroup of the Scorpius–Centaurus association.

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  • H Centauri (en)
  • V945 Centauri (pt)
  • HD 112409 (zh)
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  • HD 112409,又名CD-50 7394,SAO 240407、HR 4913,是一颗恒星,视星等为5.16,位于銀經303.83,銀緯11.66,其B1900.0坐标为赤經12h 51m 18.7s,赤緯-50° 11.66′ 25″。 (zh)
  • H Centauri (H Cen), also known as V945 Centauri, is probable triple star system located in the constellation Centaurus. From parallax measurements, it is located 113 parsecs (370 light years) from the sun. It is a member of the Lower Centaurus–Crux (LCC) subgroup of the Scorpius–Centaurus association. (en)
  • V945 Centauri (H Centauri) é um provável sistema estelar triplo na constelação de Centaurus. Tem uma magnitude aparente visual combinada de 5,16, sendo visível a olho em locais com pouca poluição luminosa. Com base em medições de paralaxe do satélite Gaia, está localizado a uma distância de 420 anos-luz (129 parsecs) da Terra. O sistema é membro do subgrupo Centaurus Inferior-Crux da , a associação OB mais próxima do Sol. (pt)
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  • H Centauri (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/V945CenLightCurve.png
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