An overview investigation of Be/Shell stars
Author:
Affiliation:
1. National Research Institute of Astronomy and Geophysics, Helwan, Egypt
Publisher
Informa UK Limited
Subject
Geophysics,Astronomy and Astrophysics
Link
https://www.tandfonline.com/doi/pdf/10.1016/j.nrjag.2012.12.004
Reference49 articles.
1. Equatorial disk formation around rotating stars due to Ram pressure confinement by the stellar wind
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