The Role of Evolutionary Age and Metallicity in the Formation of Classical Be Circumstellar Disks. I. New Candidate Be Stars in the LMC, SMC, and Milky Way-Reference-Cited by-同舟云学术

The Role of Evolutionary Age and Metallicity in the Formation of Classical Be Circumstellar Disks. I. New Candidate Be Stars in the LMC, SMC, and Milky Way

Published:2006-11-20 Issue:1 Volume:652 Page:458-471
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Wisniewski J. P.,Bjorkman K. S.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference75 articles.

1. The Small Magellanic Cloud star cluster NGC 458. A new UBVI photometric study

2. The Winds of Hot Stars in External Galaxies. III. HST UV Spectroscopy of O and B Supergiants in M31 and M33

3. Equatorial disk formation around rotating stars due to Ram pressure confinement by the stellar wind

4. A Study of π Aquarii during a Quasi‐normal Star Phase: Refined Fundamental Parameters and Evidence for Binarity

5. A Magnetically Torqued Disk Model for Be Stars

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