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astro-ph2003
The Behaviour of the Optical and X-ray Emission from Scorpius X-1
B. J. McNamara, T. E. Harrison, R. T. Zavala +11
In 1970, Hiltner & Mook reported the results of the first multiyear study of the optical emission from Sco X-1. They found that the Sco X-1 B-magnitude histograms changed from year…
astro-ph1999
Measuring the Mass of the Black Hole in GS2000+25 Using IR Ellipsoidal Variations
Dawn M. Leeber, Thomas E. Harrison, Bernard J. McNamara
Soft X-ray Transients (SXTs) are binary systems that are believed to consist of a black hole and a normal late type dwarf star which fills its Roche Lobe. We have used GRIM II on t…