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...

Bibliographic Details
Main Author:	Godon, Patrick.
Format:	Villanova Faculty Authorship
Language:	English
Published:	1995
Online Access:	http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176435

Main Author:

Godon, Patrick.

Format:

Villanova Faculty Authorship

Language:

English

Published:

1995

Online Access:

http://ezproxy.villanova.edu/login?url=https://digital.library.villanova.edu/Item/vudl:176435

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

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