Corrugations in galactic discs generated by Magellanic-type perturbers

Monthly Notices of the Royal Astronomical Society

Volumn 287, Issue 4, 1997, Pages 947-954

  Edelsohn, D J ^a,b   Elmegreen, B G ^a  

^a IBM T J WATSON RESEARCH CENTER   (United States)

^b SYRACUSE UNIVERSITY   (United States)

Author keywords

Galaxies: interactions; Galaxies: kinematics and dynamics; Galaxy: halo; Magellanic clouds; Methods: numerical

Indexed keywords

NUMERICAL METHODS;

DISK GALAXIES; GALACTIC DISKS; GALAXIES: INTERACTIONS; GALAXIES: KINEMATICS AND DYNAMICS; GALAXY:HALO; LARGE DISKS; LARGE MAGELLANIC CLOUDS; MAGELLANIC CLOUDS; METHOD: NUMERICAL; PERPENDICULAR MOTION;

GALAXIES;

EID: 0038868464     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/287.4.947     Document Type: Article

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