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• W2541407968 abstract "I discuss some of what is known and unknown about the behavior of black hole binary systems in the quiescent accretion state. Quiescence is important for several reasons: 1) the dominance of the companion star in the optical and IR wavelengths allows the binary parameters to be robustly determined - as an example, we argue that the longer proposed distance to the X-ray source GRO J1655-40 is correct; 2) quiescence represents the limiting case of an extremely low accretion rate, in which both accretion and jets can be observed; 3) understanding the evolution and duration of the quiescent state is a key factor in determining the overall demographics of X-rary binaries, which has taken on a new importance in the era of gravitational wave astronomy." @default.
• W2541407968 created "2016-11-04" @default.
• W2541407968 creator A5004465093 @default.
• W2541407968 date "2016-09-01" @default.
• W2541407968 modified "2023-09-29" @default.
• W2541407968 title "Black Hole Binaries in Quiescence" @default.
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• W2541407968 doi "https://doi.org/10.1017/s1743921317002083" @default.
• W2541407968 hasPublicationYear "2016" @default.
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