Extremely high-velocity gas in the galaxy Arp 220, revealed with ammonia absorption lines

Publications of the Astronomical Society of Japan

Volumn 57, Issue 5, 2005, Pages

  Takano, Shuro ^a,b   Nakanishi, Kouichiro ^a   Nakai, Naomasa ^c   Takano, Toshiaki ^d  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

^b GRADUATE UNIVERSITY FOR ADVANCED STUDIES   (Japan)

^c UNIVERSITY OF TSUKUBA   (Japan)

^d CHIBA UNIVERSITY   (Japan)

Author keywords

Galaxies: individual (Arp 220); Galaxies: ISM; Galaxies: starburst; Molecular processes; Radio lines: galaxies

Indexed keywords

AMMONIA;

ABSORPTION LINES; AMMONIA ABSORPTION; GALAXIES: INDIVIDUAL: ARP 220; GALAXIES: ISM; GALAXIES: STARBURSTS; GALAXY: INDIVIDUAL (ARP 220); HIGH VELOCITY; MOLECULAR PROCESS; RADIO LINES:GALAXIES; ULTRALUMINOUS INFRARED GALAXIES;

GALAXIES;

EID: 27744459429     PISSN: 00046264     EISSN: None     Source Type: Journal    
DOI: 10.1093/pasj/57.5.L29     Document Type: Article

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