The four leading arms of the Magellanic Cloud system: Evidence for interaction with Milky Way disk and halo

Astronomy and Astrophysics

Volumn 547, Issue , 2012, Pages

  Venzmer, M S ^a,b   Kerp, J ^a   Kalberla, P M W ^a  

^a UNIVERSITY OF BONN   (Germany)

^b UNIVERSITY OF GÖTTINGEN   (Germany)

Author keywords

Galaxies: interactions; Galaxy: evolution; Galaxy: halo; Magellanic Clouds

Indexed keywords

3D DATA; ALL-SKY SURVEY; ATOMIC HYDROGEN; COHERENT STRUCTURE; COLUMN DENSITY; DRAG FORCES; GALAXIES: INTERACTIONS; GALAXY: EVOLUTION; GALAXY: HALO; GAS COMPONENT; GAS CONTENT; INVERSE CORRELATION; LARGE MAGELLANIC CLOUDS; LOW-MASS; MAGELLANIC CLOUDS; MILKY WAY GALAXY; MILKY WAYS; OBJECTIVE CRITERIA; RADIAL VELOCITY; RECOGNITION ALGORITHM; VELOCITY GRADIENTS;

DRAG; HYDROGEN; IMAGE RECOGNITION; STARS; VELOCITY;

GALAXIES;

EID: 84867881176     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201118677     Document Type: Review

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