Abstract
The empirically found universal power-law form of the X-ray luminosity function for a population of high-mass X-ray binaries in galaxies can be explained by the fundamental mass-luminosity and mass-radius relations for massive stars.
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References
S. A. Eddington, The Internal Constitution of Stars (Cambridge Univ. Press, Cambridge, 1926).
H.-J. Grimm, M. R. Gilfanov, and R. A. Sunyaev, Astron. Astrophys. 391, 923 (2002).
H.-J. Grimm, M. R. Gilfanov, and R. A. Sunyaev, Mon. Not. R. Astron. Soc. (2003) (in press).
K. de Jager, The Brightest Stars (Reidel, Dordrecht, 1980; Mir, Moscow, 1984).
A. G. Masevich and A. V. Tutukov, Stellar Evolution: Theory and Observations (Nauka, Moscow, 1988).
M. Schwarzshield, Structure and Evolution of Stars (Princeton Univ. Press, Princeton, 1958).
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Translated from pis’ma v Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l}\) Zhurnal, vol. 29, No. 6, 2003, pp. 424–425.
Original Russian Text Copyright © 2003 by Postnov.
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Postnov, K.A. The universal luminosity function of binary X-ray sources in galaxies. Astron. Lett. 29, 372–373 (2003). https://doi.org/10.1134/1.1579783
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DOI: https://doi.org/10.1134/1.1579783