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G 185-32, also known by the variable star designation PY Vulpeculae, is a white dwarf in the constellation Vulpecula. Located approximately 18.3 parsecs (60 ly) distant, the stellar remnant is a ZZ Ceti variable, varying by 0.02 apparent magnitudes from the mean of 13.00.

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  • PY de la Guineueta (ca)
  • PY Vulpeculae (es)
  • G 185-32 (en)
  • PY Vulpeculae (pt)
  • PY Лисички (ru)
rdfs:comment
  • PY de la Guineueta (PY Vulpeculae) és una estrella variable (nana blanca polsant) a la constel·lació de la Guineueta. (ca)
  • G 185-32, also known by the variable star designation PY Vulpeculae, is a white dwarf in the constellation Vulpecula. Located approximately 18.3 parsecs (60 ly) distant, the stellar remnant is a ZZ Ceti variable, varying by 0.02 apparent magnitudes from the mean of 13.00. (en)
  • PY Vulpeculae (PY Vul) é uma estrela anã branca pulsante na constelação de Vulpecula. (pt)
  • PY Лисички (лат. PY Vulpeculae) — звезда, белый карлик, которая находится в созвездии Лисичка на расстоянии около 58 световых лет от нас. (ru)
  • PY Vulpeculae (PY Vul / GJ 1241 / G 185-32 / WD 1935+276)​ es una enana blanca en la constelación de Vulpecula -la zorra- situada a 60,6 años luz del Sistema Solar.​ De tipo espectral DAV4,​ su temperatura efectiva aproximada se sitúa entre 12.025 y 12.280 K.​​ Tiene una masa (M*) de 0,638 ± 0,007 masas solares, con una fracción de masa de hidrógeno de MH = 1,70 (± 0,10) × 10-4 M*.Su período de rotación estimado es de 14,5 horas.​ (es)
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  • G 185-32 (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/PYVulLightCurve.png
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absmag v
appmag 1 passband
  • J (en)
appmag 2 passband
  • H (en)
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  • K (en)
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  • DA4.0 (en)
constell
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  • J2000 (en)
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