Simulations of NGC206 and its Effects on M31 II

Details Simulations of NGC206 and its Effects on M31 II Simulations of NGC206 and its Effects on M31 II

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...19310502m&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #105.02; Bulletin of the American Astronomical Society, Vol. 30, p.1407

Astronomy and Astrophysics

Astronomy

Scientific paper

It will be shown that NGC206 is not responsible for spiral arm structure in the stellar disk in its immediate vicinity. However, it is quite likely that NGC206 does play a decisive role in the nearby dust lanes. Simulations of the stellar disk, gaseous disk, and both disks simultaneously will be presented. Parameters varied in the simulations include velocity dispersion, rotation velocity, mass of NGC206, halo-to-disk ratio, and elasticity of gaseous collisions. It is promising that results from individual simulations of the gaseous and stellar disks agree with simulations accounting for both.

Affiliated with

Also associated with

No associations

Rating

Simulations of NGC206 and its Effects on M31 II 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 Simulations of NGC206 and its Effects on M31 II, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Simulations of NGC206 and its Effects on M31 II will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-997632