High-mass X-ray binaries as a star formation rate indicator in distant galaxies
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/339/3/793/2930856/339-3-793.pdf
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1. The optical emission-line nebulae of powerful far-infrared galaxies
2. X‐Ray Emission from a Merger Remnant, NGC 7252 (the “Atoms‐for‐Peace” Galaxy)
3. The ratio of the unseen halo mass to the luminous disk mass in NGC 891
4. The Limiting Luminosity of Accreting Neutron Stars With Magnetic Fields
5. A Comparison of Ultraviolet Imaging Telescope Far‐Ultraviolet and Hα Star Formation Rates
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