Analysis of the X-ray emission of OB stars: O stars
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/1674-4527/18/i=8/a=104/pdf
Reference46 articles.
1. Long-term XMM–Newton investigation of two particle-accelerating colliding-wind binaries in NGC 6604: HD 168112 and HD 167971★
2. X-ray study of bow shocks in runaway stars
3. Ionization and thermal equilibrium models for O star winds based on time-independent radiation-driven wind theory
Cited by 6 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. 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. Analysis of the X-ray emission from OB stars III: low-resolution spectra of OB stars;Research in Astronomy and Astrophysics;2020-07-01
3. Contribution of a Non-Thermal Component to the X-Ray Emission of OB Stars;Astrophysical Bulletin;2020-04
4. Analysis of the X-ray emission of OB stars II: B stars;Research in Astronomy and Astrophysics;2019-08-01
5. A short and sudden increase of the magnetic field strength and the accompanying spectral variability in the O9.7 V star HD 54879;Monthly Notices of the Royal Astronomical Society;2019-01-18
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