Head-on Collision of Disk Sphere Galaxies

Details Head-on Collision of Disk Sphere Galaxies Head-on Collision of Disk Sphere Galaxies

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ap%26ss.301....3n&link_type=abstract

Astrophysics and Space Science, Volume 301, Issue 1-4, pp. 3-9

Astronomy and Astrophysics

Astrophysics

1

Galaxies:Interactions, Methods:Numerical

Scientific paper

Numerical simulations are performed to study the tidal effects of non-merging rapid head-on collision between a disk galaxy and a spherical galaxy. The disk consists of three components a disk, a bulge and a halo and the spherical galaxy is a Plummer model. The galaxies have the same dimensions with different mass ratios viz., 2, 1 and 0.5. They move in a rectilinear orbit with a relative velocity of 1000 km s-1.

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