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The Disk Veiling Effect of the Black Hole Low-Mass X-ray Binary A0620-00
Wan-Min Zheng, Qiaoya Wu, Jianfeng Wu +15
The optical light curves of quiescent black hole low-mass X-ray binaries often exhibit significant non-ellipsoidal variabilities, showing the photospheric radiation of the companio…
The stringent upper limit on jet power in the persistent soft state source 4U~1957+11
Thomas J. Maccarone, Arlo Osler, James C. A. Miller-Jones +5
We present extremely deep upper limits on the radio emission from 4U~1957+11, an X-ray binary that is generally believed to be a persistently accreting black hole that is almost al…
Tomography of X-ray Nova Muscae 1991: Evidence for ongoing mass transfer and stream-disc overflow
Charith S. Peris, Saeqa D. Vrtilek, James F. Steiner +9
We present a spectroscopic analysis of the black hole binary Nova Muscae 1991 in quiescence using data obtained in 2009 with MagE on the Magellan Clay telescope and in 2010 with IM…
A Dynamical Study of the Black Hole X-ray Binary Nova Muscae 1991
Jianfeng Wu, Jerome A. Orosz, Jeffrey E. McClintock +8
We present a dynamical study of the Galactic black hole binary system Nova Muscae 1991 (GS/GRS 1124-683). We utilize 72 high resolution Magellan Echellette (MagE) spectra and 72 st…