Hostname: page-component-78c5997874-94fs2 Total loading time: 0 Render date: 2024-11-19T08:31:48.320Z Has data issue: false hasContentIssue false
  • English
  • Français

The X-ray emission of E and S0 Galaxies

Published online by Cambridge University Press:  25 May 2016

G. Fabbiano
G. Fabbiano*
Affiliation:
Harvard-Smithsonian CfA, 60 Garden St., Cambridge MA 02138, USA

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.

It is well known by now that E and S0 galaxies are associated with hot, X-ray emitting gaseous halos, subject to central cooling flows, but otherwise homogeneous, which can be used to trace the galaxy potential and thus measure the total gravitational mass. Recent ASCA observations suggest that these halos have a surprisingly low metal abundance.

Type
The Interstellar Medium
Information
Symposium - International Astronomical Union , Volume 171: New Light on Galaxy Evolution , 1996 , pp. 123 - 130
Copyright
Copyright © Kluwer 1996 

References

Awaki, H. et al 1994, P. A. S. J., 46, L65.Google Scholar
Bender, R., Surma, P., Doebereiner, S., Moellenhoft, C., and Madejsky, R. 1989, Astr. Ap., 217, 35.Google Scholar
Bender, R. et al 1992, in “Structure, Dynamics, and Chemical Evolution of Elliptical Galaxies”, Danziger, I. J., Zeilinger, W. W., and Kjar, K., eds., ESO Proc. No. 45, p. 3.Google Scholar
Bender, R. and Surma, P. 1992, Astr. Ap., 258, 250.Google Scholar
Bender, R., Burstein, D., and Faber, S. M. 1992, Ap. J., 399, 462.Google Scholar
Briel, U. G., Henry, J. P., and Boehringer, H. 1992, Astr. Ap., 259, L31.Google Scholar
Buote, D., and Canizares, C. R. 1994, Ap. J., 427, 86.Google Scholar
Ciotti, L. and Pellegrini, S. 1995, M. N. R. A. S., submitted.Google Scholar
David, L. P., Jones, C., Forman, W., and Daines, S. 1994, Ap. J., 428, 544.CrossRefGoogle Scholar
Eskridge, P. B., Fabbiano, G., and Kim, D.-W. 1995a, Ap. J. Suppl., 97, 141.Google Scholar
Eskridge, P. B., Fabbiano, G., and Kim, D.-W. 1995b, Ap. J., 442, 523.Google Scholar
Eskridge, P. B., Fabbiano, G., and Kim, D.-W. 1995c, Ap. J., in press.Google Scholar
Fabbiano, G. 1989, Ann. Rev. Ast. Ap., 27, 87.Google Scholar
Fabbiano, G. 1995, in “Fresh Views on Elliptical Galaxies”, Buzzoni, A., ed., Pub. of A. Soc. P., in press.Google Scholar
Fabbiano, G., Kim, D.-W., and Trinchieri, G. 1992, Ap. J. Suppl., 80, 531.CrossRefGoogle Scholar
Fabbiano, G., Gioia, I. M., and Trinchieri, G. 1989, Ap. J., 347, 127.Google Scholar
Fabbiano, G., Kim, D.-W., and Trinchieri, G. 1994, Ap. J., 429, 94.CrossRefGoogle Scholar
Fabbiano, G., and Schweizer, F. 1995, Ap. J., in press.Google Scholar
Fabbiano, G., Trinchieri, G., and VanSpeybroeck, L. 1987, Ap. J., 316, 127.Google Scholar
Faber, S. M. 1973, Ap. J., 179, 731.CrossRefGoogle Scholar
Fabricant, D., and Gorenstein, P. 1983, Ap. J., 267, 535.CrossRefGoogle Scholar
Forman, Jones, C. and Tucker, W., 1985, Ap. J., 293, 102.Google Scholar
Forman, W., Schwarz, J., Jones, C., Liller, W., and Fabian, A. C. 1979, Ap. J., 234, L27.CrossRefGoogle Scholar
Hernquist, L., and Barnes, J. E. 1991, Nature, 354, 210.Google Scholar
Killeen, N.E.D. and Bicknell, G.V. 1988, Ap. J., 325, 169.Google Scholar
Kim, D.-W., and Fabbiano, G. 1995, Ap. J., 441, 182.Google Scholar
Kim, D.-W., Fabbiano, G., Mackie, G., and Norman, C. 1995, Ap. J., submitted.Google Scholar
Matsushita, K. et al 1994, Ap. J., 436, L41.Google Scholar
Meyer, J. 1991, Adv. Space Res., 11, 269.Google Scholar
Miyata, E., Tsunemi, H., Pisarski, R., and Kissel, S. E. 1994, P. A. S. J., 46, L101.Google Scholar
Pellegrini, S. 1994, Astr. Ap., 292, 395.Google Scholar
Pellegrini, S. and Fabbiano, G. 1994, Ap. J., 429, 105.CrossRefGoogle Scholar
Phillips, K. J. H., Pike, C. D., Lang, J., Watanabe, T., and Zarro, D. M. 1994, Proc. of Kofu Symp., NRO Report No. 360, p. 301.Google Scholar
Stiavelli, M. 1992 in “Structure, Dynamics, and Chemical Evolution of Elliptical Galaxies”, Danziger, I. J., Zeilinger, W. W., and Kjar, K., eds., ESO Proc. No. 45, p. 303.Google Scholar
Trinchieri, G., and di Serego Alighieri, S. 1991, A. J., 101, 1647.Google Scholar
Trinchieri, G., and Fabbiano, G. 1991, Ap. J., 382, 82.Google Scholar
Trinchieri, G., Fabbiano, G., and Canizares, C. R. 1986, Ap. J., 310, 637.Google Scholar
Trinchieri, G, Kim, D.-W., Fabbiano, G., and Canizares, C. R., 1994, Ap. J., 428, 555.CrossRefGoogle Scholar
White, N. E. et al 1994, P. A. S. J., 46, L97.Google Scholar