The Infrared Counterpart of the X-Ray Nova XTE J1720-318

Publications of the Astronomical Society of Japan

Volumn 55, Issue 6, 2003, Pages

  Nagata, Tetsuya ^a   Kato, Daisuke ^a   Baba, Daisuke ^a   Nishiyama, Shogo ^a   Nagayama, Takahiro ^a   Nagashima, Chie ^a   Kurita, Mikio ^a   Sato, Shuji ^a   Kato, Taichi ^b   Uemura, Makoto ^b   Yamaoka, Hitoshi ^c   Monard, Berto ^d   Ita, Yoshifusa ^e   Matsunaga, Noriyuki ^e   Nakajima, Yasushi ^f   Tamura, Motohide ^f   Nakaya, Hidehiko ^f   Sugitani, Koji ^g  

^a NAGOYA UNIVERSITY   (Japan)

^b KYOTO UNIVERSITY   (Japan)

^c KYUSHU UNIVERSITY   (Japan)

^d Bronberg Observatory   (South Africa)

^e UNIVERSITY OF TOKYO   (Japan)

^f NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^g NAGOYA CITY UNIVERSITY   (Japan)

Author keywords

Accretion, accretion disks; Infrared: stars; Stars: activity; Stars: individual (XTE J1720 318)

Indexed keywords

LIGHT EXTINCTION;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; INFRARED LIGHT; INFRARED: STAR; LIGHT CURVES; OBSERVATION PERIOD; STAR: ACTIVITY; STAR: INDIVIDUAL (XTE J1720-318); STARS: INDIVIDUAL: PROXIMA CENTAURI; X-RAY TRANSIENTS;

STARS;

EID: 1442303686     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/55.6.l73     Document Type: Article

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