DISK-LOSS AND DISK-RENEWAL PHASES IN CLASSICAL Be STARS. II. CONTRASTING WITH STABLE AND VARIABLE DISKS
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/786/i=2/a=120/pdf
Reference71 articles.
1. Equatorial disk formation around rotating stars due to Ram pressure confinement by the stellar wind
2. Magnetically Fed Hot Star Keplerian Disks with Slow Outflow
3. Spectroscopic atlas of Hαand Hβin a sample of northern Be stars
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