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

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

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