UBVR photometry and rotation of late-type galaxies - NGC 959, 1156, 1160, 6643, and 7292

Details UBVR photometry and rotation of late-type galaxies - NGC 959, 1156, 1160, 6643, and 7292 UBVR photometry and rotation of late-type galaxies - NGC 959, 1156, 1160, 6643, and 7292

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991azh....68..909e&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 68, Sept.-Oct. 1991, p. 909-917. In Russian.

Astronomy and Astrophysics

Astronomy

4

Astronomical Photometry, Galactic Rotation, Ubv Spectra, Angular Velocity, Brightness Distribution, Color, Density Distribution

Scientific paper

Brightness and color distribution profiles for five late-type galaxies obtained from observations with the magnetic-focusing image tube are presented. Rotation curves and density distribution models are derived as well. A comparison of photometric and kinematic data shows that the stellar population content changes slowly with the galactocentric distance. Density depression in the central parts of the disk is needed to explain the rotation curves of three out of the five galaxies under consideration.

Affiliated with

Also associated with

No associations

Rating

UBVR photometry and rotation of late-type galaxies - NGC 959, 1156, 1160, 6643, and 7292 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 UBVR photometry and rotation of late-type galaxies - NGC 959, 1156, 1160, 6643, and 7292, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UBVR photometry and rotation of late-type galaxies - NGC 959, 1156, 1160, 6643, and 7292 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1875576