The environmental density and the bulge-to-disk ratio of disk galaxies in the Local Supercluster.

Details The environmental density and the bulge-to-disk ratio of disk galaxies in the Local Supercluster. The environmental density and the bulge-to-disk ratio of disk galaxies in the Local Supercluster.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996apl%26c..33..139g&link_type=abstract

Astrophysical Letters and Communications, Vol. 33, Nos. 1 - 5, p. 139 - 141

Astronomy and Astrophysics

Astrophysics

Local Supercluster: Disk Galaxies

Scientific paper

Relying on several samples of disk galaxies for which a detailed photometric bulge/disk decomposition has been given in the literature, the authors have investigated on the relation between the bulge-to-disk light ratio (B/D) and the environmental density. For nearby (z < 0.01) galaxies, they provide a well-defined three-dimensional characterization of the local galaxy density. Unlike previous claims, B/D appears to be unrelated to the galaxy absolute magnitude.

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