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Bulk Velocities, Chemical Composition, and Ionization Structure of the X‐Ray Shocks in WR 140 near Periastron as Revealed by theChandraGratings

  • Published:2005-08-10 Issue:1 Volume:629 Page:482-498
  • ISSN:0004-637X
  • Container-title:The Astrophysical Journal
  • language:en
  • Short-container-title:ApJ

Author:

Pollock A. M. T.,Corcoran Michael F.,Stevens Ian R.,Williams P. M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 93 articles. 订阅此论文施引文献 订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

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

2. X-ray plasma flow and turbulence in the colliding winds of WR140;Monthly Notices of the Royal Astronomical Society;2023-11-27

3. Inverse-Compton cooling of thermal plasma in colliding-wind binaries;Monthly Notices of the Royal Astronomical Society;2023-09-18

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

5. Understanding the physical state of hot plasma formed through stellar wind collision in WR140 using high-resolution X-ray spectroscopy;Monthly Notices of the Royal Astronomical Society;2022-05-10
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