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Populations of X-ray Binaries and the Dynamical History of their Host Galaxies

Published online by Cambridge University Press:  05 March 2013

Kinwah Wu
Kinwah Wu*
Affiliation:
Research Centre for Theoretical Astrophysics, School of Physics, University of Sydney, NSW 2006, Australia, and Mullard Space Science Laboratory, University College London, Holmbury St Mary, Surrey RH5 6NT, United Kingdom; [email protected]
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Abstract

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The observed luminosity distributions of X-ray sources indicate the presence of several populations of X-ray binaries in the nearby galaxies. Each population has its formation and evolutionary history, depending on the host environment. The features seen in the log N(>S)–log S curves for different types of galaxies and for different galactic components can be reproduced by a birth–death model, in which the lifespans of the binaries are inversely proportional to their X-ray brightness. Conversely, the dynamical history of a galaxy can be inferred from the luminosity distributions of its X-ray binary populations.

Keywords

galaxies: evolutionX-ray: binaries
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 18 , Issue 4 , 2001 , pp. 443 - 450
Copyright
Copyright © Astronomical Society of Australia 2001

References

Blanton, E. L., Sarazin, C. L., & Irwin, J. A. 2001, ApJ, 552, 106 Google Scholar
de Loore, C. W. H., & Doom, C. 1992, Structure and Evolution of Single and Binary Stars (Dordrecht: Kluwers Academic Press)CrossRefGoogle Scholar
Fabbiano, G. 1995, in X-ray Binaries, eds. W. H. G. Lewin J. van Paradijs, & E. P. J. van den Heuvel (Cambridge: Cambridge University Press), 390 Google Scholar
Fabbiano, G., Zezas, A., & Murray, S. S. 2001, ApJ, 554, 1035 Google Scholar
Finoguenov, A., & Jones, C. 2001, ApJ, 547, L107 Google Scholar
Garcia, M. R., et al. 2000, ApJ, 537, L23 CrossRefGoogle Scholar
Irwin, J. A., Bregman, J. N., & Sarazin, C. L. 2001, ApJ, submitted (astro-ph/01074–93)Google Scholar
Johnston, H. M., & Verbunt, F. 1996, A&A, 312, 80 Google Scholar
Kraft, R. P., et al. 2000, ApJ, 531, L9 Google Scholar
Landau, L. D., & Lifshitz, E. M. 1971, The Classical Theory of Fields (Oxford: Pergamon Press)Google Scholar
Matsumoto, H., et al. 2001, ApJ, 547, L25 Google Scholar
Paczynski, B. 1967, Acta Astron., 17, 287 Google Scholar
Pence, W. D., Snowden, S. L., Mukai, K., & Kuntz, K. D. 2001, ApJ, submitted (astro-ph/0107133)Google Scholar
Roberts, T. R., & Warwick, R. S. 2000, MNRAS, 315, 98 CrossRefGoogle Scholar
Sambruna, R. M., et al. 2001, ApJ, 546, L9 Google Scholar
Sarazin, C. L., Irwin, J. A., & Bregman, J. N. 2000, ApJ, 544, L101 Google Scholar
Schechter, P. 1976, ApJ, 203, 297 Google Scholar
Shirey, R., et al. 2001, A&A, 365, L195 Google Scholar
Skumanich, A. 1972, ApJ, 171, 565 Google Scholar
Supper, R., et al. 1997, A&A, 317, 328 Google Scholar
Tennant, A. F., Wu, K., Ghosh, K. K., Kolodziejczak, J. J., & Swartz, D. A. 2001, ApJ, 549, L43 Google Scholar
Verbunt, F., & Zwaan, C., 1981, A&A, 100, L7 Google Scholar
Wang, Q. D., Immler, S., & Pietsch, W. 1999, ApJ, 523, 121 CrossRefGoogle Scholar
Weisskopf, M. C., Tananbaum, H. D., Van Speybroeck, L. P., & O'Dell, S. L. 2000, Proc. SPIE, 4012, 2 CrossRefGoogle Scholar
Wu, K. 1997, in Accretion Phenomena and Related Outflows, eds. D. T. Wickramasinghe G. V. Bicknell, & L. Ferrario, ASP Conf. Ser., 121, 283 Google Scholar
Wu, K., Tennant, A. F., Swartz, D. A., Ghosh, K. K., & Hunstead, R. W. 2001, ApJ, submittedGoogle Scholar