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  Bright end of the luminosity function of high-mass X-ray binaries: contributions of hard, soft and supersoft sources

Sazonov, S., & Khabibullin, I. (2017). Bright end of the luminosity function of high-mass X-ray binaries: contributions of hard, soft and supersoft sources. Monthly Notices of the Royal Astronomical Society, 466(1), 1019-1051. doi:10.1093/mnras/stw3113.

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 Creators:
Sazonov, S., Author
Khabibullin, I.1, Author              
Affiliations:
1High Energy Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159881              

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Language(s): eng - English
 Dates: 2017-04
 Publication Status: Published in print
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1093/mnras/stw3113
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Title: Monthly Notices of the Royal Astronomical Society
  Abbreviation : Mon. Not. Roy. Astron. Soc.
Source Genre: Journal
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Pages: - Volume / Issue: 466 (1) Sequence Number: - Start / End Page: 1019 - 1051 Identifier: ISSN: 0035-8711
ISSN: 1365-8711