Hostname: page-component-76fb5796d-zzh7m Total loading time: 0 Render date: 2024-04-25T09:47:31.641Z Has data issue: false hasContentIssue false
  • English
  • Français

The Circumstellar Matter of Cygnus X-3

Published online by Cambridge University Press:  25 May 2016

S. Kitamoto  and
K. Kawashima
S. Kitamoto
Affiliation:
Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1, Machikaneyama-cho, Toyonaka, Osaka, 560, JAPAN
K. Kawashima
Affiliation:
Department of Earth and Space Science, Graduate School of Science, Osaka University, 1-1, Machikaneyama-cho, Toyonaka, Osaka, 560, JAPAN

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

X-ray source in Cyg X-3 is embedded in the photo-ionized circumstellar gas. Recombination edges and emission lines were detected by ASCA observation (Kawashima, Kitamoto 1996; Liedahl, Paerels 1996). The strength of the Kα line and the recombination edge are simply determined by the atomic process. Therefore, the comparison of observed these intensities is a good tool to study the Cyg X-3 system.

Type
Session 3: Diagnostics of High Gravity Objects with X- and Gamma Rays
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 356 - 357
Copyright
Copyright © Kluwer 1998 

References

Kawashima, K., Kitamoto, S. 1996, PASJ, 48, L113 Google Scholar
Liedahl, D. A., Paerels, F. 1996, ApJ, 468, L33 Google Scholar
Kitamoto, S, Miyamoto, S., Matsui, W., Inoue, H., 1987, PASJ, 39, 259 Google Scholar