Hot boundary layers in symbiotic binaries ax persei and ci cygni.

Accretion disk boundary layer models are calculated for the symbiotic binaries AX Per and CI Cyg, using a time-dependent numerical code. Hot boundary layers are found with temperatures above 10 K, assuming for the accreting star a mass M* = 0.5 M0 and a radius R * = 0.2 R0. However, choosing a large...

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Bibliographic Details
Main Author: Godon, Patrick.
Format: Villanova Faculty Authorship
Published: 1995
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