Rapid optical fluctuations in the black hole binary V4641 sagittarii

Publications of the Astronomical Society of Japan

Volumn 54, Issue 5, 2002, Pages

  Uemura, Makoto ^a   Kato, Taichi ^a   Ishioka, Ryoko ^a   Tanabe, Kenji ^b   Kiyota, Seiichiro ^c   Monard, Berto ^d   Stubbings, Rod ^e   Nelson, Peter ^e   Richards, Tom ^f   Bailyn, Charles ^g   Santallo, Roland ^h  

^a KYOTO UNIVERSITY   (Japan)

^b OKAYAMA UNIVERSITY OF SCIENCE   (Japan)

^c VSOLJ   (Japan)

^d Bronberg Observatory   (South Africa)

^e Woodridge Observatory ^*

^f Woodridge Observatory   (Australia)

^g YALE UNIVERSITY   (United States)

^h Faaa   (France)

Author keywords

Accretion, accretion disks; Stars: binaries: close; Stars: individual (V4641 Sagittarii)

Indexed keywords

BLACK HOLES; GRAVITATION; POWER SPECTRUM; STARS;

ACCRETION: ACCRETION DISKS; BLACK HOLES; OPTICAL EMISSIONS; OPTICAL FLUCTUATION; OPTICAL FLUX; POWER-SPECTRA; SHORT-TERM VARIATIONS; STAR: INDIVIDUAL (V4641 SAGITTARII); STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:BINARIES CLOSE;

LIGHT EMISSION;

EID: 0036455856     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/54.5.L79     Document Type: Article

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