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• W3100141822 abstract "We report optical spectroscopic observations of the low-mass X-ray binary GRO J1655-40 during outbursts in 1994 August-September and in 1996 June. The spectra show emission and absorption lines from the accretion disk surrounding the X-ray source, which have enabled us to measure the motion of the black hole candidate in this system. It is the first time among black hole candidates that an emission-line radial velocity curve is seen in phase with the expected motion of the primary. The projected radial velocity semiamplitude determined for the primary (KX = 76.2±7.5 km s-1), combined with estimates of the projected radial velocity semiamplitude of the companion star from previous observations (KC=228.2±3.0 km s-2), yields a 95% confidence limit, derived purely from kinematics, of MX > 5.1 M☉ for the mass of the compact object in GRO J1655-40, confirming its black hole nature." @default.
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• W3100141822 date "1998-03-10" @default.
• W3100141822 modified "2023-09-26" @default.
• W3100141822 title "Measuring the Motion of the Black Hole in GRO J1655−40" @default.
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• W3100141822 doi "https://doi.org/10.1086/311225" @default.
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