The Effect of Porosity on X‐Ray Emission‐Line Profiles from Hot‐Star Winds-Reference-Cited by-同舟云学术

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The Effect of Porosity on X‐Ray Emission‐Line Profiles from Hot‐Star Winds

Published:2006-09 Issue:1 Volume:648 Page:565-571
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Owocki Stanley P.,Cohen David H.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference26 articles.

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

2. ROSATPSPC Observations of 27 Near–Main‐Sequence B Stars

3. Wind signatures in the X-ray emission-line profiles of the late-O supergiant Orionis

4. Two-dimensional simulations of the line-driven instability in hot-star winds

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1. X-ray Emission of Massive Stars and Their Winds;Handbook of X-ray and Gamma-ray Astrophysics;2024

2. Survey of X-Rays from Massive Stars Observed at High Spectral Resolution with Chandra;The Astrophysical Journal;2023-08-29

3. Disentangling physics and chemistry in AGB outflows: revealing degeneracies when adding complexity;Faraday Discussions;2023

4. Theory and Diagnostics of Hot Star Mass Loss;Annual Review of Astronomy and Astrophysics;2022-08-18

5. X-Ray Emission of Massive Stars and Their Winds;Handbook of X-ray and Gamma-ray Astrophysics;2022

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