High-resolution X-ray spectroscopy of bright O-type stars
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/372/1/313/5783658/mnras0372-0313.pdf
Reference43 articles.
1. Lower mass loss rates in O-type stars: Spectral signatures of dense clumps in the wind of two Galactic O4 stars
2. Optically thick clumps – not the solution to the Wolf-Rayet wind momentum problem?
3. The effects of coronal regions on the X-ray flux and ionization conditions in the winds of OB supergiants and Of stars
4. [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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