Possible formation scenarios for the giant H I envelope around the NGC 4490/4485 system

Monthly Notices of the Royal Astronomical Society

Volumn 297, Issue 4, 1998, Pages 1015-1020

  Clemens, M S ^a   Alexander, P ^a   Green, D A ^a  

^a CAVENDISH LABORATORY   (United Kingdom)

Author keywords

Galaxies: evolution; Galaxies: individual: NGC 4485; Galaxies: individual: NGC 4490; Galaxies: interactions; Radio lines: galaxies

Indexed keywords

SUPERNOVAE;

GALAXIES: INDIVIDUALS; GALAXIES: INTERACTIONS; GALAXY EVOLUTION; GALAXY: INDIVIDUAL: NGC 4485; GALAXY: INDIVIDUAL: NGC 4490; MASS LOSS; NEUTRAL HYDROGEN; RADIO LINES:GALAXIES;

GALAXIES;

EID: 0007154541     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01510.x     Document Type: Article

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