On the peculiarities of evolutionary history of EHB objects in binary systems with hot subdwarf companions

Details On the peculiarities of evolutionary history of EHB objects in binary systems with hot subdwarf companions On the peculiarities of evolutionary history of EHB objects in binary systems with hot subdwarf companions

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..353..149p&link_type=abstract

Stellar Evolution at Low Metallicity: Mass Loss, Explosions, Cosmology ASP Conference Series, Vol. 353, Proceedings of the Confe

Mathematics

Probability

Scientific paper

It has been shown quite recently ( teauthor{MA} teyear{MA}, teauthor{MO} teyear{MO}) that dB stars - extreme horizontal branch (EHB) objects in high probability all belong to binary systems. We study in detail the mass and angular momentum loss in the giant progenitors of sdB stars in an attempt to clarify why binarity must be a crucial factor in producing EHB objects.

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