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V Sagittae

Variable star in the constellation Sagitta From Wikipedia, the free encyclopedia

V Sagittae
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V Sagittae or V Sge is a cataclysmic variable in the constellation Sagitta. The system is composed of a main sequence star of about 3.3 solar masses and a Wolf-Rayet star[3] of about 0.9 solar masses.[7] V Sge is the only super soft X-ray source nonmagnetic cataclysmic variable found so far.

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A visual band light curve for V Sagittae, adapted from Šimon and Mattei (1999)[8]
Quick Facts Observation data Epoch J2000 Equinox J2000, Constellation ...

Material from the larger star is accreting onto the WR star at an exponentially increasing rate, generating a huge stellar wind. The doubling time for the accretion rate, and hence for the system luminosity, is about 89±11 years.[5] It is predicted that the system will erupt as a nova some time between 2067 and 2099, at which point it will become one of the brightest stars in the sky.[7][9]

Component A was long thought to be a white dwarf, but the primary component show similarities with a Wolf-Rayet stars and the model with a white dwarf and its accretion disk does not explain many aspects of the system, including orbital period variations and mass loss from the primary.[3]

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