A result of interacting galaxies: numerical simulation of ring galaxy formation.

Details A result of interacting galaxies: numerical simulation of ring galaxy formation. A result of interacting galaxies: numerical simulation of ring galaxy formation.

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acaps..16....7l&link_type=abstract

Acta Astrophys. Sin., Vol. 16, No. 1, p. 7 - 14

Astronomy and Astrophysics

Astrophysics

Ring Galaxies: Numerical Simulations, Ring Galaxies: Formation

Scientific paper

Ring galaxy formation is studied through the numerical simulation of the collision of two galaxies involving a target galaxy and an intruder galaxy. In distinction with Toomre's work the author uses spiral structure as the distribution function of test stars of the target galaxy disk. This results in the simulated ring structure bearing closer resemblance to that of real ring galaxies than Toomre's simulation does.

Affiliated with

Also associated with

No associations

Rating

A result of interacting galaxies: numerical simulation of ring galaxy formation. 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 A result of interacting galaxies: numerical simulation of ring galaxy formation., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A result of interacting galaxies: numerical simulation of ring galaxy formation. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-967338