Outburst and Post-Outburst Active Phase of the Black Hole X-Ray Binary V4641 Sagittarii in 2002

Publications of the Astronomical Society of Japan

Volumn 56, Issue SPEC. ISS. 1, 2004, Pages

  Uemura, Makoto ^a   Kato, Taichi ^a   Ishioka, Ryoko ^a   Tanabe, Kenji ^b   Torii, Ken'ichi ^c   Santallo, Roland ^d   Monard, Berto ^e   Markwardt, Craig B ^f   Swank, Jean H ^g   Sault, Robert J ^h   Macquart, Jean Pierre ⁱ   Linnolt, Michael ^j   Kiyota, Seiichiro ^k   Stubbings, Rod ^j   Nelson, Peter ^l   Richards, Tom ^m   Bailyn, Charles ⁿ   West, Doug ^o   Masi, Gianluca ^j   Miyashita, Atsushi ^p   Sano, Yasuo ^q   Scarmato, Toni ^j   more..

^a KYOTO UNIVERSITY   (Japan)

^b OKAYAMA UNIVERSITY OF SCIENCE   (Japan)

^c RIKEN   (Japan)

^d Southern Stars Observatory   (French Polynesia)

^e Bronberg Observatory   (South Africa)

^f Bldg 142   (United States)

^g NASA GODDARD SPACE FLIGHT CENTER   (United States)

^h CSIRO   (Australia)

ⁱ UNIVERSITY OF GRONINGEN   (Netherlands)

^j Center for Balcony Astrophysics ^*  (Italy)

^k Center for Balcony Astrophysics   (Japan)

^l RMB 2493   (Australia)

^m Woodridge Observatory   (Australia)

ⁿ YALE UNIVERSITY   (United States)

^o West Skies Observatory   (United States)

^p Seikei High School   (Japan)

^q VSOLJ   (Japan)

more..

Author keywords

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

Indexed keywords

BLACK HOLES; GRAVITATION; OPTICAL CORRELATION; C (PROGRAMMING LANGUAGE);

ACCRETION: ACCRETION DISKS; ACTIVE PHASIS; BLACK HOLES; LIGHT CURVES; RAPID VARIATION; STAR: INDIVIDUAL (V4641 SAGITTARII); STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS:BINARIES CLOSE; X-RAY WAVELENGTHS; X-RAYS: BINARIES; ACCRETION; ACCRETION DISCS;

STARS;

EID: 1942440913     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/56.sp1.s61     Document Type: Article

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