Orbital motion and mass flow in the interacting binary Be star HR 2142
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1538-3873/95/i=567/a=311/pdf
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3. Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries?;The Astrophysical Journal;2019-11-11
4. Spectro-interferometric observations of a sample of Be stars;Astronomy & Astrophysics;2019-01
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