Chemical abundances in the secondary star of the black hole binary V4641 Sagittarii (SAX J1819.3-2525)

Publications of the Astronomical Society of Japan

Volumn 58, Issue 3, 2006, Pages 595-604

  Sadakane, Kozo ^a   Arai, Akira ^a   Aoki, Wako ^b   Arimoto, Nobuo ^b   Takada Hidai, Masahide ^c   Ohnishi, Takashi ^d   Tajitsu, Akito ^b   Beers, Timothy C ^e   Iwamoto, Nobuyuki ^f   Tominaga, Nozomu ^g   Umeda, Hideyuki ^g   Maeda, Keiichi ^g   Nomoto, Ken'ichi ^g  

^a OSAKA KYOIKU UNIVERSITY   (Japan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^c TOKAI UNIVERSITY   (Japan)

^d Nagoya Science Museum   (Japan)

^e MICHIGAN STATE UNIVERSITY   (United States)

^f JAPAN ATOMIC ENERGY AGENCY   (Japan)

^g UNIVERSITY OF TOKYO   (Japan)

Author keywords

Stars: abundances; Stars: binaries; Stars: individual (v4641 Sagittarii); Stars: micro quasars; Stars: X rays

Indexed keywords

GRAVITATION; SPECTROSCOPIC ANALYSIS; SUPERNOVAE;

BLACK HOLES; CHEMICAL ABUNDANCE; SECONDARY STARS; SPECTROSCOPIC STUDIES; STAR: INDIVIDUAL (V4641 SAGITTARII); STAR: MICRO-QUASAR; STARS ABUNDANCES; STARS: BINARIES; STARS: INDIVIDUAL: PROXIMA CENTAURI; STARS: X-RAY;

MAGNESIUM COMPOUNDS;

EID: 33746582712     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/58.3.595     Document Type: Article

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