GRO J1655-40: Measuring the mass of the BH from the optical emission lines

Details GRO J1655-40: Measuring the mass of the BH from the optical emission lines GRO J1655-40: Measuring the mass of the BH from the optical emission lines

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aipc..431..335s&link_type=abstract

Accretion processes in astrophysical systems: Some like it hot! - eigth astrophysics conference. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astrophysics

X-Ray Binaries, Black Holes, Accretion And Accretion Disks, Visible

Scientific paper

The optical spectra of the X-ray binary GRO J1655-40, taken during
periods of high optical brightness, can provide important information on
the kinematics of the system, on the mass of the primary (confirming its
nature of BH), on the size and physical structure of the disk, and on
the effects of X-ray irradiation.

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