The luminosity of galactic components and morphological segregation

Details The luminosity of galactic components and morphological segregation The luminosity of galactic components and morphological segregation

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989aj.....98..798s&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 98, Sept. 1989, p. 798-805. Research supported by the Direccion General de Investiga

Mathematics

Logic

18

Disk Galaxies, Galactic Bulge, Luminosity, Galactic Radiation, Morphology, Statistical Distributions

Scientific paper

The luminosities of the bulge and disk components of disk galaxies are analyzed, and the possible correlation of these luminosities with morphological type and local density is explored. Galaxies of different types are found to be located in distinct bands in the bulge-to-disk luminosity ratio vs total luminosity diagram, allowing the determination of the typical bulge luminosity function of disk galaxies of different types from their respective total luminosity functions, along with a better characterization of morphological segregation among disk galaxies. No evidence for any bulge luminosity segregation is found, and disks appear to be less luminous with increasing local density.

Affiliated with

Also associated with

No associations

Rating

The luminosity of galactic components and morphological segregation 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 luminosity of galactic components and morphological segregation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The luminosity of galactic components and morphological segregation will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-761080