The outburst radial velocity curve of X-ray Nova Scorpii 1994 (= GRO J1655-40): A reduced mass for the black hole?

Monthly Notices of the Royal Astronomical Society

Volumn 304, Issue 4, 1999, Pages 839-844

  Phillips, S N ^a   Shahbaz, T ^a   Podsiadlowski, Ph ^a  

^a UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

Accretion, accretion discs; Binaries: close; Stars: individual: X ray Nova Sco 1994 (GRO J1655 40); X rays: stars

Indexed keywords

BLACK HOLES; SUPERNOVAE; VELOCITY;

ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; BLACK HOLES; RADIAL VELOCITY CURVES; RADIAL VELOCITY DATUM; REANALYSIS; REDUCED MASS; STAR: INDIVIDUAL: X-RAY NOVA SCO 1994 (GRO J1655-40); STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAY:STARS;

GRAVITATION;

EID: 0001544019     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02357.x     Document Type: Article

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