The frequency of occurrence of disk galaxies with a two-humped curve of rotation

Details The frequency of occurrence of disk galaxies with a two-humped curve of rotation The frequency of occurrence of disk galaxies with a two-humped curve of rotation

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..210z&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, March 1989, p. 210-215. In Russian. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Disk Galaxies, Galactic Bulge, Galactic Rotation, Brightness Distribution, Density Distribution, Stellar Luminosity

Scientific paper

If the density distribution in disks and bulges of galaxies follows the luminosity distribution of these components, then a significant part of the galaxies must have a two-humped curve of rotation which passes through a local minimum in the inner part of the galaxy. It is shown that the VK galaxies must amount to a significant part of all disk galaxies. Consideration is given to a simplified two-component model of the galaxy in which the density distribution in disks and bulges corresponds to the standard law of the brightness distribution of these components.

Affiliated with

Also associated with

No associations

Rating

The frequency of occurrence of disk galaxies with a two-humped curve of rotation 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 The frequency of occurrence of disk galaxies with a two-humped curve of rotation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The frequency of occurrence of disk galaxies with a two-humped curve of rotation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1528075