Atomic gas far away from the Virgo cluster core galaxy NGC 4388. A possible link to isolated star formation in the Virgo cluster?

Astronomy and Astrophysics

Volumn 406, Issue 2, 2003, Pages 427-434

  Vollmer, B ^a   Huchtmeier, W ^a  

^a MAX PLANCK INSTITUT FÜR RADIOASTRONOMIE   (Germany)

Author keywords

Galaxies: individual: NGC 4388; Galaxies: interactions; Galaxies: ISM; Galaxies: kinematics and dynamics

Indexed keywords

ATMOSPHERIC PRESSURE; CLOUDS; COMPUTER SIMULATION; DENSITY OF GASES; GASES; GRAVITATION; KINEMATICS; VELOCITY; WIND;

ATOMIC GAS; NUMERICAL RAM PRESSURE SIMULATION; STAR-FORMING CLOUD; VIRGO CLUSTER CORE GALAXY;

GALAXIES;

EID: 0042204202     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20030516     Document Type: Article

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