The optical light curves of Cygnus X-2 (V1341 Cyg) and the mass of its neutron star
Open Access
- 1 May 1999
- journal article
- research article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 305 (1) , 132-142
- https://doi.org/10.1046/j.1365-8711.1999.t01-1-02420.x
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This publication has 33 references indexed in Scilit:
- X-ray irradiation in low-mass binary systemsMonthly Notices of the Royal Astronomical Society, 1999
- On the Formation of Low-Mass Black Holes in Massive Binary StarsThe Astrophysical Journal, 1996
- Properties of the massive X-ray binary 4U 1700 - 37 = HD 153919The Astrophysical Journal, 1992
- Approximations to the radii of Roche lobesThe Astrophysical Journal, 1983
- Confirmation of a 9.8-day period of Cygnus X-2Publications of the Astronomical Society of the Pacific, 1980
- The halo population X-ray source Cygnus X-2The Astrophysical Journal, 1979
- Ellipsoidal light variations and masses of X-ray binariesThe Astrophysical Journal, 1975
- A spectroscopic analysis of HZ Her.The Astrophysical Journal, 1974
- Optical properties of HZ Her.The Astrophysical Journal, 1974
- On the Optical Search for the X-Ray Sources CYG X-1 and CYG X-2The Astrophysical Journal, 1967