Origin of the counterrotating gas in NGC 1596

Monthly Notices of the Royal Astronomical Society

Volumn 370, Issue 3, 2006, Pages 1565-1572

  Chung, Aérée ^a   Koribalski, Bärbel ^b   Bureau, Martin ^c   Van Gorkom, J H ^a  

^a Howard Hughes Medical Institute   (United States)

^b CSIRO   (Australia)

^c UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

Galaxies: individual: NGC 1596; Galaxies: interactions; Galaxies: ISM; Galaxies: kinematics and dynamics; Galaxies: spiral; Galaxies: stellar content

Indexed keywords

GALAXIES; GASES; STARS;

COUNTER ROTATING; GALAXIES: INDIVIDUALS; GALAXIES: INTERACTIONS; GALAXIES: ISM; GALAXIES: KINEMATICS AND DYNAMICS; GALAXIES: SPIRALS; GALAXY: INDIVIDUAL: NGC 1596; GALAXY:STELLAR CONTENT; IONIZED GAS; VELOCITY GRADIENTS;

IONIZATION OF GASES;

EID: 33746521213     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10579.x     Document Type: Article

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