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- V Puppis (V Pup / HD 65818 / HR 3129) es un sistema estelar variable en la constelación de Puppis, la popa del Argo Navis. De magnitud aparente media +4,45, se encuentra a unos 1165 años luz de distancia del sistema solar. (es)
- V Puppis (V Pup) is a star system in the constellation Puppis. Its apparent magnitude is 4.41. There is a binary star system at the center with a B1 dwarf orbiting a B3 subgiant star. They have an orbital period of 1.45 days and a distance of only 15 solar radii apart. However, the system moves back and forth, indicating that there is a massive object orbiting them with a period around 5.47 years. Based on the mass of the object, its lack of a visible spectrum, and circumstellar matter in the system with many heavy elements (as would be produced by a past supernova in the system), it is probably a black hole. However, a follow-up study could not confirm this object, but found signs that there may be a third object which is fainter than the other components. In addition to the main system, more distant components have been reported: B, at magnitude 11.5 and separation 6.2", C, at magnitude 13.2 and separation 18.9", D, at magnitude 9.88 and separation 39", and E, at magnitude 13 and separation from D of 10.4". (en)
- HD 65818, nota anche come V Puppis, è una stella binaria di magnitudine 4,45 situata nella costellazione della Poppa. Dista 1000 anni luce dal sistema solare ed è una variabile a eclisse. (it)
- V Puppis är en förmörkelsevariabel av Beta Lyrae-typ (EB/SD) i stjärnbilden Akterskeppet. Stjärnan varierar mellan visuell magnitud +4,35 och 4,92 med en period av 1,4544859 dygn. (sv)
- 船尾座V，又名CD-48 3349，HD 65818、SAO 219226、HR 3129，是船尾座的一颗恒星，视星等为4.41，位于銀經263.48，銀緯-10.28，其B1900.0坐标为赤經7h 55m 21.9s，赤緯-48° -10.28′ 25″。 (zh)
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- 8512 (xsd:nonNegativeInteger)
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- 4.410000 (xsd:double)
- (en)
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- V Pup Aa (en)
- V Pup Ab (en)
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- 6500 (xsd:integer)
- 12600 (xsd:integer)
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- 7.300000 (xsd:double)
- 14 (xsd:integer)
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- 4.590000 (xsd:double)
- 5.480000 (xsd:double)
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- 24000 (xsd:integer)
- 26000 (xsd:integer)
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- V Puppis (V Pup / HD 65818 / HR 3129) es un sistema estelar variable en la constelación de Puppis, la popa del Argo Navis. De magnitud aparente media +4,45, se encuentra a unos 1165 años luz de distancia del sistema solar. (es)
- HD 65818, nota anche come V Puppis, è una stella binaria di magnitudine 4,45 situata nella costellazione della Poppa. Dista 1000 anni luce dal sistema solare ed è una variabile a eclisse. (it)
- V Puppis är en förmörkelsevariabel av Beta Lyrae-typ (EB/SD) i stjärnbilden Akterskeppet. Stjärnan varierar mellan visuell magnitud +4,35 och 4,92 med en period av 1,4544859 dygn. (sv)
- 船尾座V，又名CD-48 3349，HD 65818、SAO 219226、HR 3129，是船尾座的一颗恒星，视星等为4.41，位于銀經263.48，銀緯-10.28，其B1900.0坐标为赤經7h 55m 21.9s，赤緯-48° -10.28′ 25″。 (zh)
- V Puppis (V Pup) is a star system in the constellation Puppis. Its apparent magnitude is 4.41. There is a binary star system at the center with a B1 dwarf orbiting a B3 subgiant star. They have an orbital period of 1.45 days and a distance of only 15 solar radii apart. However, the system moves back and forth, indicating that there is a massive object orbiting them with a period around 5.47 years. Based on the mass of the object, its lack of a visible spectrum, and circumstellar matter in the system with many heavy elements (as would be produced by a past supernova in the system), it is probably a black hole. However, a follow-up study could not confirm this object, but found signs that there may be a third object which is fainter than the other components. (en)
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- V Puppis (es)
- HD 65818 (it)
- V Puppis (en)
- V Puppis (sv)
- 船尾座V (zh)
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