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X-ray Properties of Spiral Galaxies

Published online by Cambridge University Press:  26 May 2016

Roberto Soria
Roberto Soria*
Affiliation:
Mullard Space Science Laboratory, University College London, Holmbury St Mary, Surrey RH5 6NT, UK; [email protected]

Abstract

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X-ray studies of nearby spiral galaxies with star formation allow us to investigate temperature and spatial distribution of the hot diffuse plasma, and to carry out individual and statistical studies of different classes of discrete sources (low- and high-mass X-ray binaries, Supernova remnants, supersoft and ultra-luminous sources). In particular, we briefly review the different models proposed to explain the ultra-luminous sources. We can then use the X-ray properties of a galaxy to probe its star formation history. We choose the starburst spiral M83 to illustrate some of these issues.

Type
Part 2 The Data Base of High Energy Astrophysics
Information
Symposium - International Astronomical Union , Volume 214: High Energy Processes and Phenomena in Astrophysics , 2003 , pp. 59 - 69
Copyright
Copyright © Astronomical Society of the Pacific 2003 

References

Begelman, M. C. 2002, 568, L97 Google Scholar
Blanton, E. L., Sarazin, C. L., & Irwin, J. A. 2001, ApJ, 552, 106 Google Scholar
Calzetti, D., Bohlin, R. C., Kinney, A. L., Storchi-Bergmann, T., & Heckman, T. M. 1995, ApJ, 443, 136 CrossRefGoogle Scholar
Condon, J. J., Yin, Q. F., Thuan, T. X., & Boiler, Th. 1998, AJ, 116, 2682 CrossRefGoogle Scholar
de Vaucouleurs, G., de Vaucouleurs, A., Buta, H. G., Paturel, G., & Fouque, P. 1991, in the Third General Catalogue of Bright Galaxies Google Scholar
Di Stefano, R., & Kong, A. K. H. 2003, ApJ, submitted Google Scholar
Ebisuzaki, T. et al. 2001, ApJ, 562, L19 Google Scholar
Fabbiano, G., & Shapley, A. 2002, ApJ, 565, 908 CrossRefGoogle Scholar
Fabrika, S., & Mescheryakov, A. 2001, in “Galaxies and their Constituents at the Highest Angular Resolutions”, Proceedings of the IAU Symposium 205 (Manchester, 15–18 August 2000), p. 268 (astro-ph/0103070) Google Scholar
Giacconi, R., et al. 2002, ApJS, 139, 369 Google Scholar
King, A. R., Davies, M. B., Ward, M. J., Fabbiano, G., & Elvis, M. 2001, ApJ, 552, L109 Google Scholar
Kubota, A., Mizuno, T., Makishima, K., Fukazawa, Y., Kotoku, J., Ohnishi, T., & Tashiro, M. 2001, ApJ, 547, L119 CrossRefGoogle Scholar
Kulkarni, S. R., Hut, P., & McMillan, S. L. W. 1993, Nature, 364, 421 Google Scholar
La Parola, V., Peres, G., Fabbiano, G., Kim, D. W., & Bocchino, F. 2001, ApJ, 556, 47 CrossRefGoogle Scholar
Liedahl, D. A., Sako, M., Wojdowski, P. S., Paerels, F., & Kahn, S. M. 2000, Revista Mexicana de Astronomia y Astrofisica, 9, 40 Google Scholar
Madau, P., & Rees, M. J. 2001, ApJ, 551, 27 Google Scholar
Makishima, et al. 2000, ApJ, 535, 632 Google Scholar
Margon, B., Lampton, M., & Cruddace, R. 1974, ApJ, 190, 285 Google Scholar
Matsumoto, H., Tsuru, T. G., Koyama, K., Awaki, H., Canizares, C. R., Kawai, N., Matsushita, S., & Kawabe, R. 2001, ApJ, 457, L25 Google Scholar
Miller, M. C., & Hamilton, D. P. 2002, ApJ, 576, 894 CrossRefGoogle Scholar
Pakull, M. W., & Mirioni, L. 2002, in the proceedings of the symposium “New Visions of the X-ray Universe in the XMM-Newton and Chandra Era”, 26–30 November 2001, ESTEC, The Netherlands (astro-ph/0202488) Google Scholar
Roberts, T. P., & Warwick, R. S. 2000, MNRAS, 315, 98 Google Scholar
Roberts, T. P., Warwick, R. S., Ward, M. J., & Murray, S. S. 2002, MNRAS, in press (astro-ph/0208196) Google Scholar
Roberts, T. P., Goad, M. R., Ward, M. J., Warwick, R. S., O'Brien, P. T., Lira, P., & Hands, A. D. P. 2001, MNRAS, 325, L7 Google Scholar
Sarazin, C. L., Irwin, J. A., & Bregman, J. N. 2000, ApJ, 544, L101 Google Scholar
Shaviv, N. J. 1998, ApJ, 494, L193 CrossRefGoogle Scholar
Shaviv, N. J. 2001, MNRAS, 326, 126 CrossRefGoogle Scholar
Soria, R., & Wu, K., 2002, A&A, 384, 99 Google Scholar
Soria, R., & Wu, K., 2003, A&A, submitted Google Scholar
Sigurdsson, S., & Hernquist, L. 1993, Nature, 364, 423 Google Scholar
Strickland, D. K., Colbert, E. J. M., Heckman, T. M., Weaver, K. A., Dahlem, , & Stevens, M., Stevens, I.R. 2001, ApJ, 560, 707 CrossRefGoogle Scholar
Swartz, D., Ghosh, K., Suleimanov, V., Tennant, A., & Wu, K. 2002, ApJ, in press (astro-ph/0203487) Google Scholar
Tennant, A. F., Wu, K., Ghosh, K. K., Kolodziejczak, J. J., & Swartz, D. A. 2001, ApJ, 549, L43 CrossRefGoogle Scholar
Valinia, A., & Marshall, F. E. 1998, ApJ, 505, 134 Google Scholar
Wu, K. 2001, PASA, 18, 443 Google Scholar
Zezas, A., & Fabbiano, G. 2002, ApJ, 577, 726 Google Scholar