Identifying stars of mass >150 M⊙ from their eclipse by a binary companion
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnrasl/article-pdf/425/1/L91/6283816/425-1-L91.pdf
Reference44 articles.
1. THE LOW-MASS INITIAL MASS FUNCTION IN THE 30 DORADUS STARBURST CLUSTER
2. TOWARD AN ACCURATE DETERMINATION OF PARAMETERS FOR VERY MASSIVE STARS: THE ECLIPSING BINARY LMC-SC1-105
3. Bonanos A. Z. 2012 in Richards, M.T., Hubeny, I., eds, Proc. IAU Symp. 282 27
4. GEMINI/GMOS SEARCH FOR MASSIVE BINARIES IN THE IONIZING CLUSTER OF 30 DOR
5. Generic Spectrum and Ionization Efficiency of a Heavy Initial Mass Function for the First Stars
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1. Probingintermediate-mass black holes in M87 through multiwavelength gravitational wave observations;Monthly Notices of the Royal Astronomical Society;2020-05-16
2. Eclipsing Stellar Binaries in the Galactic Center;The Astrophysical Journal;2017-12-20
3. The Evolution of Compact Binary Star Systems;Living Reviews in Relativity;2014-05-05
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