Transitions to and from stable discs in cataclysmic variable stars
作者： Brian Warner
DOI: 10.1007/BF00658170
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摘要: The observational properties of Z Cam stars, nova-like variables and nova remnants are discussed in terms the disc instability model. effects irradiation on secondary star, giving rise to high low states mass transfer, inner disc, suppressing or greatly reducing instability, used explain light curves VY Scl stars. Irradiation may also play a part producing amplitude modulations brightness nova-likes time scales tens days.
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