Hostname: page-component-7bb8b95d7b-wpx69 Total loading time: 0 Render date: 2024-09-12T02:22:29.526Z Has data issue: false hasContentIssue false
  • English
  • Français

X-ray AGN; The View from ASCA

Published online by Cambridge University Press:  30 March 2016

Hideyo Kunieda
Hideyo Kunieda*
Affiliation:
Department of Physics Nagoya University Chikusa, Nagoya, 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.

ASCA capability of X-ray imaging spectroscopy up to 10 keV. allows us to examine the emission and absorption feature from AGN. Warm absorber, low energy lines and broad iron K lines are confirmed from Sy I’s. High sensitivity in broad energy band makes it possible to distinguish multiple components emerged by different processes. Detection of X-rays from faint sources tells us various galaxies may harbor AGN sometimes with obscuration tori. They might have considerable contribution to CXB.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 10: Highlights of Astronomy. As presented at the XXIInd General Assembly of the IAU, 1994 , 1995 , pp. 513 - 516
Copyright
Copyright © Kluwer 1995

References

Fabian, et al., PASJ, 46, L55–L58, (1994a)Google Scholar
Fabian, et al., Ap. J Letter (in press) (1994b)Google Scholar
Makishima, et al. PASJ, 46, L77–L80 (1994)Google Scholar
Serlemitsos, et al. Submitted to PASJ (1994)Google Scholar
Stella, et al., Proc. “Iron line Diagnostics in X-ray Sources (1990)” p. 230 Google Scholar
Ueno, et al., PASJ, 46, L71–L75 (1994)Google Scholar