Classification of paired galaxies into groups differing in physical and kinematic properties

Details Classification of paired galaxies into groups differing in physical and kinematic properties Classification of paired galaxies into groups differing in physical and kinematic properties

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978sva....22..148m&link_type=abstract

(Astronomicheskii Zhurnal, vol. 55, Mar.-Apr. 1978, p. 249-261.) Soviet Astronomy, vol. 22, Mar.-Apr. 1978, p. 148-154. Transla

Astronomy and Astrophysics

Astrophysics

Astrophysics, Galactic Clusters, Ubv Spectra, Astronomical Models, Galactic Evolution, Galactic Structure, Kinematics, Radial Velocity, Stellar Motions

Scientific paper

Forty-seven pairs of galaxies, most of which are close or interacting, have been considered. All these pairs may be divided into three separate groups according to specific relations between the (U-B) color indices of their members. Comparison of spectral types, absolute magnitudes, radial velocities, and other characteristics of the pair members support the reality of existence of such groups. Evidence is given that the groups considered differ in origin or evolution.

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