On the formation of tails and bridges in interacting galaxies

Details On the formation of tails and bridges in interacting galaxies On the formation of tails and bridges in interacting galaxies

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985basi...13..363n&link_type=abstract

Astronomical Society of India, Bulletin, vol. 13, Dec. 1985, p. 363-371.

Statistics

Computation

2

Celestial Mechanics, Galactic Structure, Gravitational Effects, Interacting Galaxies, Boundary Value Problems, Computational Astrophysics, Galaxies, Orbit Perturbation

Scientific paper

Interacting galaxies produce peculiar features like tails, bridges, and counterarms of various sizes and shapes. Numerical experiments have been performed to investigate how the formation of tails and bridges depends on mass ratio of the two interacting galaxies. Results indicate that tail formation is favored when the mass ratio mu is close to unity. When mu is much less than one, the tail appears to be shorter and thinner than in the case when mu is about unity. As a result of the encounter, a sharp decrease in the density of the main galaxy at the tidal radius is numerically observed.

Affiliated with

Also associated with

No associations

Rating

On the formation of tails and bridges in interacting galaxies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with On the formation of tails and bridges in interacting galaxies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the formation of tails and bridges in interacting galaxies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1160793