Superwind-driven intense H2 emission in NGC 6240

Publications of the Astronomical Society of Japan

Volumn 52, Issue 4, 2000, Pages 563-576

  Ohyama, Youichi ^a   Yoshida, Michitoshi ^a   Takata, Tadafumi ^a   Imanishi, Masatoshi ^a,b   Usuda, Tomonori ^a   Saito, Yoshihiko ^c   Taguchi, Hiroko ^d   Ebizuka, Noboru ^e   Iwamuro, Fumihide ^f   Motohara, Kentaro ^f   Taguchi, Tomoyuki ^f   Hata, Ryuji ^f   Maihara, Toshinori ^f   Iye, Masanori ^a   Sasaki, Toshiyuki ^a   Kosugi, George ^a   Ogasawara, Ryusuke ^a   Noumaru, Junichi ^a   Mizumoto, Yoshihiko ^a   Yagi, Masafumi ^a   Chikada, Yoshihiro ^a   more..

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b UNIVERSITY OF HAWAII   (United States)

^c UNIVERSITY OF TOKYO   (Japan)

^d TOKYO GAKUGEI UNIVERSITY   (Japan)

^e NATIONAL INSTITUTE OF INFORMATION AND COMMUNICATIONS TECHNOLOGY   (Japan)

^f KYOTO UNIVERSITY   (Japan)

Author keywords

Galaxies: Individual (NGC 6240); Galaxies: Interactions; Galaxies: Intergalactic medium; Infrared: Galaxies; Infrared: Spectra; Shock waves

Indexed keywords

GALAXIES; VELOCITY; SHOCK WAVES;

BLUE-SHIFTED; GALAXIES INTERGALACTIC MEDIUM; GALAXIES: INDIVIDUALS; GALAXIES: INTERACTIONS; GALAXY: INDIVIDUAL (NGC 6240); INFRARED GALAXIES; INFRARED SPECTRUM; K BANDS; PEAK POSITION; SHOCK-WAVES; LINE RATIOS;

SHOCK WAVES; GALAXIES;

EID: 0034355189     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/52.4.563     Document Type: Article

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