X‐Ray Spectral Study of the Photoionized Stellar Wind in Vela X‐1-Reference-Cited by-同舟云学术

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X‐Ray Spectral Study of the Photoionized Stellar Wind in Vela X‐1

Published:2006-11 Issue:1 Volume:651 Page:421-437
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Watanabe Shin,Sako Masao,Ishida Manabu,Ishisaki Yoshitaka,Kahn Steven M.,Kohmura Takayoshi,Nagase Fumiaki,Paerels Frederik,Takahashi Tadayuki

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference37 articles.

1. The mass of the neutron star in Vela X-1

2. The shadow wind in high-mass X-ray binaries

3. Hydrodynamic simulations of stellar wind disruption by a compact X-ray source

4. Enhanced winds and tidal streams in massive X-ray binaries

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2. Spectral Modeling of the Supersoft X-Ray Source CAL87 Based on Radiative Transfer Codes;The Astrophysical Journal;2023-12-21

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5. Photoionization of ground and excited states of Cr VIII with Rydberg series analysis of resonances involved;Indian Journal of Physics;2023-09-27

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