The Effects of Clumps in Explaining X‐Ray Emission Lines from Hot Stars-Reference-Cited by-同舟云学术

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The Effects of Clumps in Explaining X‐Ray Emission Lines from Hot Stars

Published:2008-08-20 Issue:2 Volume:683 Page:1052-1062
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:Astrophysical Journal

Author:

Cassinelli J. P.,Ignace R.,Waldron W. L.,Cho J.,Murphy N. A.,Lazarian A.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference65 articles.

1. Mass loss from very luminous OB stars and the Cygnus superbubble

2. Infrared photometry and mass loss rates for OBA supergiants and Of stars

3. Lower mass loss rates in O-type stars: Spectral signatures of dense clumps in the wind of two Galactic O4 stars

4. Quantitative Spectroscopy of O Stars at Low Metallicity: O Dwarfs in NGC 346

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1. Analysis of X-Ray Emission from OB Stars. IV. About X-Ray Emission from Inhomogeneous Winds of OB Stars;Research in Astronomy and Astrophysics;2023-09-27

2. 3D RMHD simulations of jet-wind interactions in high-mass X-ray binaries;Astronomy & Astrophysics;2022-05

3. The Colliding Winds of WR 25 in High-resolution X-Rays;The Astrophysical Journal;2021-07-01

4. A Deep Exposure in High Resolution X-Rays Reveals the Hottest Plasma in the ζ Puppis Wind;The Astrophysical Journal;2020-04-15

5. Unraveling the Nature of the Deeply Embedded Wolf–Rayet Star WR 121a;The Astrophysical Journal;2020-03-11

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