Dynamic Processes in Be Star Atmospheres. VI. Simultaneous X‐Ray, Ultraviolet, and Optical Variations in λ Eridani-Reference-Cited by-同舟云学术

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Dynamic Processes in Be Star Atmospheres. VI. Simultaneous X‐Ray, Ultraviolet, and Optical Variations in λ Eridani

Published:1997-05-20 Issue:1 Volume:481 Page:479-488
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Smith Myron A.,Murakami T.,Ezuka H.,Anandarao B. G.,Chakraborty A.,Corcoran M. F.,Hirata R.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/481/i=1/a=479/pdf

Reference37 articles.

1. Long term X-ray variability studies of OB-type stars

2. Bolton, C. T. & Stefl, S. 1990, in Angular Momentum and Mass Loss for Hot Stars, ed. L. Willson & R. Stalio (Dordrecht: Kluwer), 191

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1. Modeling of the Wind/Disk Outflow from Be Stars;Universe;2021-09-23

2. Winds from fast rotating stars;Monthly Notices of the Royal Astronomical Society;2021-01-11

3. Be Star Disks: Powered by a Nonzero Central Torque;The Astrophysical Journal;2020-12-23

4. Searching for the presence of a weak magnetic field in the Be star λ Eri using FORS 2 spectropolarimetric time series;Astronomische Nachrichten;2017-10

5. An overview investigation of Be/Shell stars;NRIAG Journal of Astronomy and Geophysics;2012-12

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