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BV Centauri is a cataclysmic variable binary star in the constellation Centaurus. It is a dwarf nova, and undergoes rapid increases in brightness that are recurrent with a mean period of 150 days. This period seems to have increased in the last few decades. During quiescence, its visual apparent magnitude is about 13, with variations of a few tenths of magnitude over an orbit due to differences in the star's visible surface area (ellipsoidal variability), brightening to a maximum magnitude of 10.7 during outbursts. From its luminosity, it is estimated that the system is about 500 parsecs (1,600 ly) away from Earth. A Gaia parallax of 2.81 mas has been measured, corresponding to about 360 pc.

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  • BV Centauri (en)
  • BV Centauri (pt)
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  • BV Centauri is a cataclysmic variable binary star in the constellation Centaurus. It is a dwarf nova, and undergoes rapid increases in brightness that are recurrent with a mean period of 150 days. This period seems to have increased in the last few decades. During quiescence, its visual apparent magnitude is about 13, with variations of a few tenths of magnitude over an orbit due to differences in the star's visible surface area (ellipsoidal variability), brightening to a maximum magnitude of 10.7 during outbursts. From its luminosity, it is estimated that the system is about 500 parsecs (1,600 ly) away from Earth. A Gaia parallax of 2.81 mas has been measured, corresponding to about 360 pc. (en)
  • BV Centauri é uma estrela binária variável cataclísmica na constelação de Centaurus. É uma , apresentando aumentos rápidos de luminosidade que são recorrentes com um período médio de 150 dias, que parece ter aumentado nas últimas décadas. Durante o estado quieto, sua magnitude aparente visual é de aproximadamente 13, com variações de alguns décimos ao longo de uma órbita devido a diferenças na área visível das estrelas, aumentando até um máximo de 10,7 nas erupções. Medições de paralaxe pelo satélite astrométrico Gaia determinaram que o sistema está a uma distância de aproximadamente 361 parsecs (1 178 anos-luz) da Terra, um valor menor que a estimativa indireta anterior de 500 parsecs, baseada na sua luminosidade. (pt)
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  • BV Centauri (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/BVCenLightCurve.png
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  • G5-G8IV-V (en)
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