A dynamical model for galactic bulges

Details A dynamical model for galactic bulges A dynamical model for galactic bulges

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985apj...295..314j&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 295, Aug. 15, 1985, p. 314-323.

Astronomy and Astrophysics

Astrophysics

22

Bulging, Dynamic Models, Galactic Bulge, Galactic Structure, Stellar Motions, Axisymmetric Bodies, Disk Galaxies, Equations Of Motion, Integral Equations, Oblate Spheroids, Potential Fields

Scientific paper

A dynamical model for the bulges of disk galaxies is described. The models are axisymmetric and are based on a distribution function of the two isolating integrals of motion, energy and angular momentum. The bulge models have nonzero total angular momentum and are spatially truncated by an energy cutoff. An externally imposed disk potential field has also been included.

Affiliated with

Also associated with

No associations

Rating

A dynamical model for galactic bulges 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 dynamical model for galactic bulges, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A dynamical model for galactic bulges will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-752961