The mass ratio of Nova Muscae 1991

Authors: Casares J.; Martin E.L.; Charles P.A.; Molaro P.; Rebolo R.

Source: New Astronomy, Volume 1, Number 4, March 1997 , pp. 299-310(12)

Publisher: Elsevier

Keywords: [Physical Astronomy Classification Scheme] 97.10.G; [Physical Astronomy Classification Scheme] 97.60.L; [Physical Astronomy Classification Scheme] 97.80.F; [Physical Astronomy Classification Scheme] 97.80.J; Accretion; accretion disks; Binaries; close; Black hole physics; X-rays; stars; Stars; individual; Nova Mus 1991

Language: English

Document Type: Research article

DOI: http://dx.doi.org/10.1016/S1384-1076(96)00022-X

Affiliations: 1: University of Oxford, Department of Physics, Nuclear Physics, Laboratory, Keble Road, Oxford OX1 3RH, UK

Publication date: 1997-03-01

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• By this author: Casares J. ;  Martin E.L. ;  Charles P.A. ;  Molaro P. ;  Rebolo R.

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