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Populations of Massive X-Ray Binaries

Published online by Cambridge University Press:  22 February 2018

Ignacio Negueruela
Ignacio Negueruela*
Affiliation:
Universidad de Alicante, Spain

Abstract

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The population of massive X-ray binaries in a galaxy can provide important constraints on its recent history of star formation. However, further knowledge of the Galactic population and formation mechanisms is needed before deeper inferences can be made for other galaxies.

Resumen

Resumen

La población de binarias masivas de rayos X en una galaxia nos informa sobre su historia redoute do formación estelar. Sin embargo, es necesario un conocimiento más profundo de la población de estos sistemas en la Vía Láctea y sus mecanismos de formación para poder explotar esta información.

Keywords

BinariesClose — PulsarsGeneral — X-RaysBinaries
Type
The Contributed Papers
Information
International Astronomical Union Colloquium , Volume 194: Compact binaries in the galaxy and beyond , 2004 , pp. 55 - 56
Copyright
Copyright © Instituto de astronomia/revista mexicana de astronomίa y astrofίsica 2004

References

Delgado-Martí, H., Levine, A.M., Pfahl, E., & Rappaport, S.A. 2001, ApJ 546, 455 CrossRefGoogle Scholar
van den Heuvel, E.P.J., & van Paradijs, J. 1997, ApJ 483, 399 CrossRefGoogle Scholar
Negueruela, I., & Сое, M.J. 2002, A&A 385, 517 Google Scholar
Negueruela, I., Israel, G. L., Marco, A., et al. 2003, A&A 397, 739 Google Scholar
Okazaki, A.T.. & Negueruela, I. 2001. A&A 377, 161 Google Scholar
Pfahl, E., Rappaport, S. Podsiadlowski, P., & Spruit, H. 2002. ApJ 574, 364 CrossRefGoogle Scholar
Podsiadlowski, Ph.. Langer, N.. Poelarends, A.J.T., et al. 2003. ApJ, in pressGoogle Scholar
Reig, P., & Roche, P. 1999, MNRAS 306, 100 CrossRefGoogle Scholar