The black hole transient Nova Scorpii 1994 ( = GRO J1655 - 40): Orbital ephemeris and optical light curve

Monthly Notices of the Royal Astronomical Society

Volumn 286, Issue 4, 1997, Pages

  Van Der Hooft, F ^a   Groot, P J ^a   Shahbaz, T ^b   Augusteijn, T ^c   Casares, J ^b   Dieters, S ^d   Greenhill, J ^e   Hill, K ^e   Scheers, L H A ^a   Naber, R M ^a   De Jong, J A ^a   Charles, P A ^b   Van Paradijs, J ^a,d  

^a UNIVERSITY OF AMSTERDAM   (Netherlands)

^b UNIVERSITY OF OXFORD   (United Kingdom)

^c EUROPEAN SOUTHERN OBSERVATORY   (Chile)

^d UNIVERSITY OF ALABAMA IN HUNTSVILLE   (United States)

^e UNIVERSITY OF TASMANIA   (Australia)

Author keywords

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

Indexed keywords

BLACK HOLES; GRAVITATION;

ACCRETION: ACCRETION DISKS; BINARIES: CLOSE; BLACK HOLES; HOLE TRANSIENTS; LIGHT CURVES; ORBITALS; SECONDARY STARS; STAR: INDIVIDUAL: NOVA SCO 1994 (GRO J1655 - 40); STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAY:STARS;

STARS;

EID: 0001876856     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/286.4.L43     Document Type: Article

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