High-mass X-ray binaries as a star formation rate indicator in distant galaxies

Grimm, H.-J.; Gilfanov, M.; Sunyaev, R.

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High-mass X-ray binaries as a star formation rate indicator in distant galaxies

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Grimm, H.-J.
High Energy Astrophysics, MPI for Astrophysics, Max Planck Society;

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Gilfanov, M.
High Energy Astrophysics, MPI for Astrophysics, Max Planck Society;

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Sunyaev, R.
High Energy Astrophysics, MPI for Astrophysics, Max Planck Society;

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Grimm, H.-J., Gilfanov, M., & Sunyaev, R. (2003). High-mass X-ray binaries as a star formation rate indicator in distant galaxies. Monthly Notices of the Royal Astronomical Society, 339(3), 793-809. Retrieved from http://www.blackwell-synergy.com/links/doi/10.1046/j.1365-8711.2003.06224.x/abs/.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-B9D0-0

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