作者: B. Paczyński , J. Ziółkowski , A. Żytkow
DOI: 10.1007/978-94-010-3405-0_30
关键词: Stars 、 Astrophysics 、 Mass transfer 、 Scale (ratio) 、 Physics 、 Envelope (waves) 、 Binary number 、 Outflow 、 Roche lobe 、 Component (thermodynamics)
摘要: We show that the mass outflow from more massive component of a close binary fills up its Roche lobe, may take place on dynamical time-scale if this has deep con-vective envelope. suggest outbursts U Geminorum-type stars might be related to phenomenon.