New clues on outburst mechanisms and improved spectroscopic elements of the black hole binary V4641 Sagittarii

Monthly Notices of the Royal Astronomical Society

Volumn 363, Issue 3, 2005, Pages 882-890

  Lindstrom C ^a   Griffin, J ^a   Kiss, L L ^a,e   Uemura, M ^b,c   Derekas, A ^a,d   Meszaros Sz ^e   Szekely P ^e  

^a UNIVERSITY OF SYDNEY   (Australia)

^b UNIVERSITY OF CONCEPCIÓN   (Chile)

^c KYOTO UNIVERSITY   (Japan)

^d UNIVERSITY OF NEW SOUTH WALES   (Australia)

^e UNIVERSITY OF SZEGED   (Hungary)

Author keywords

Black hole physics; Stars: individual: V4641 Sagittarii; X rays: binaries

Indexed keywords

BLACK HOLES; GRAVITATION;

BLACK HOLE PHYSICS; BLACK HOLES; BLUE-SHIFTED; EMISSION LINES; MULTIPLE COMPONENTS; PHOTOMETRICS; SPECTRA'S; STAR: INDIVIDUAL: V4641 SAGITTARII; STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAYS: BINARIES;

STARS;

EID: 27344445609     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09483.x     Document Type: Article

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