Hostname: page-component-cd9895bd7-q99xh Total loading time: 0 Render date: 2024-12-26T04:11:35.807Z Has data issue: false hasContentIssue false

Recent Ginga Results on Extragalactic X-Ray Sources

Published online by Cambridge University Press:  30 March 2016

Y. Tanaka*
Affiliation:
Institute of Space and Astronautical Science3-1-1 Yoshinodai, Sagamihara, Kanagawa-ken 229, Japan

Abstract

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.

Many active galactic nuclei (AGNs) have been observed from Ginga, and their spectra as well as the time variations have been studied. Study of the sky brightness fluctuation has given a new result related to the cosmic X-ray background.

Type
Joint Discussions
Copyright
Copyright © Kluwer 1992

References

REFERENCES

Awaki, H. et al. (1990), Nature, 346, 544.Google Scholar
Awaki, H. (1991), ISAS Research Note, RN 473.Google Scholar
Cavallo, G. and Rees, M.J. (1978), M.N.R.A.S., 183, 359.Google Scholar
Fabian, A.C. (1979), Proc. Royal Soc. London, A, 366, 449.Google Scholar
Fabian, A.C. et al. (1990), M.N.R.A.S., 242, 14.Google Scholar
Hayashida, K. (1990), ISAS Research Note, RN 466.Google Scholar
Makino, F. (1989), Astrophys. J. Letters, 347, L9.Google Scholar
Matsuoka, M. et al. (1990), Astrophys. J., 361, 440.Google Scholar
Marshall, F.E. et al. (1980), Astrophys. J., 235, 4.Google Scholar
Pounds, K.A. et al. (1990), Nature, 344, 132.Google Scholar
Remillard, R.A. et al. (1991), Nature, 350, 589.Google Scholar
Tanaka, Y., (1990), Proc. Workshop on “Iron Line Diagnostics in X-Ray Sources”, Varenna, 1990.Google Scholar
Tanaka, Y., Proceedings of this Joint Discussion.Google Scholar
Terasawa, N. (1991), Astrophys. J. Letters, 378, L11.Google Scholar
Warwick, R.S. and Stewart, G.C. (1989), Proc. 23rd ESLAB Symp., Bologna, 1989, 2, p. 727.Google Scholar