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HD 96919, also known by its Bayer designation of z2 Carinae and the variable star designation of V371 Carinae, is a blue supergiant star in the constellation Carina. It lies near the Carina Nebula and at a comparable distance. V371 Car is an α Cyg variable, erratically pulsating and changing brightness by a few hundredths of a magnitude. Periods of 10–80 days have been identified. It shows unusual emission lines in its spectrum, and high-velocity absorption (HVA) events, temporary spectral features that are thought to indicate localised regions of enhanced mass loss.

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rdf:type
rdfs:label
  • HD 96919 (en)
  • HD 96919 (it)
  • 261 Carinae (pt)
  • V371 Киля (ru)
  • HD96919 (uk)
  • 船底座V371 (zh)
rdfs:comment
  • HD 96919 è una stella supergigante azzurra di magnitudine 5,15 situata nella costellazione della Carena. Dista 5528 anni luce dal sistema solare. (it)
  • 261 Carinae (z² Carinae) é uma estrela na direção da Carina. Possui uma ascensão reta de 11h 08m 34.01s e uma declinação de −61° 56′ 49.8″. Sua magnitude aparente é igual a 5.11. Considerando sua distância de 5525 anos-luz em relação à Terra, sua magnitude absoluta é igual a −6.04. Pertence à classe espectral B9Ia. É uma estrela variável Alpha Cygni. (pt)
  • V371 Киля (V371 Carinae, z2 Киля, z2 Carinae) — бело-голубой сверхгигант спектрального класса В9lae в созвездии Киля. Удалён от Земли на 1920 парсек. Звезда является переменной типа Альфы Лебедя и меняет свой блеск в интервале от +5,12 до +5,19. Невооружённым глазом звезда наблюдается только в ясную погоду и зоркими людьми. (ru)
  • HD96919 — хімічно пекулярна зоря спектрального класу A0, що має видиму зоряну величину в смузі V приблизно 5,1.Вона розташована на відстані близько 5528,1 світлових років від Сонця. (uk)
  • 船底座V371,又名CP-61 2075,HD 96919、SAO 251286、HR 4338,是船底座的一颗恒星,视星等为5.13,位于銀經291.15,銀緯-1.45,其B1900.0坐标为赤經11h 4m 24.1s,赤緯-61° -1.45′ 20″。 (zh)
  • HD 96919, also known by its Bayer designation of z2 Carinae and the variable star designation of V371 Carinae, is a blue supergiant star in the constellation Carina. It lies near the Carina Nebula and at a comparable distance. V371 Car is an α Cyg variable, erratically pulsating and changing brightness by a few hundredths of a magnitude. Periods of 10–80 days have been identified. It shows unusual emission lines in its spectrum, and high-velocity absorption (HVA) events, temporary spectral features that are thought to indicate localised regions of enhanced mass loss. (en)
foaf:name
  • V371 Carinae (en)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Carina_constellation_map.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/V371CarLightCurve.png
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