Prevalence of SED Turndown among Classical Be Stars: Are All Be Stars Close Binaries?
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ab48e7/pdf
Reference177 articles.
1. Binaries among B2-B5 IV, V absorption and emission stars
2. Stellar parameters and H α line profile variability of Be stars in the BeSOS survey
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