Abbott Wave–triggered Runaway in Line‐driven Winds from Stars and Accretion Disks-Reference-Cited by-同舟云学术

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Abbott Wave–triggered Runaway in Line‐driven Winds from Stars and Accretion Disks

Published:2002-01 Issue:1 Volume:564 Page:385-394
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Feldmeier Achim,Shlosman Isaac

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/564/i=1/a=385/pdf

Reference40 articles.

1. The theory of radiatively driven stellar winds. I - A physical interpretation

2. The theory of radiatively driven stellar winds. II - The line acceleration

3. The origin of stellar winds - Subatmospheric nonthermal storage modes versus radiation pressure

4. X-ray emission from near-main-sequence B stars

5. [ITAL]Chandra[/ITAL] Detection of Doppler-shifted X-Ray Line Profiles from the Wind of ζ Puppis (O4 [CLC]f[/CLC])

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1. Radiation-pressure Waves and Multiphase Quasar Outflows;The Astrophysical Journal;2019-11-01

2. Time-dependent radiation-driven winds;Monthly Notices of the Royal Astronomical Society;2018-10-01

3. The accretion environment of supergiant fast X-ray transients probed withXMM-Newton;Astronomy & Astrophysics;2017-12

4. Towards a Unified View of Inhomogeneous Stellar Winds in Isolated Supergiant Stars and Supergiant High Mass X-Ray Binaries;Space Science Reviews;2017-03-07

5. Mass loss from hot massive stars;The Astronomy and Astrophysics Review;2008-12

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