Double galaxies with Markaryan components

Details Double galaxies with Markaryan components Double galaxies with Markaryan components

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981pazh....7....3k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 7, Jan. 1981, p. 3-8.) Soviet Astronomy Letters, vol. 7, Jan.-Feb. 1981, p. 1-4. Trans

Astronomy and Astrophysics

Astronomy

11

Galactic Clusters, Galaxies, Stellar Evolution, Luminosity, Markarian Galaxies, Radial Velocity, Star Distribution, Ultraviolet Astronomy

Scientific paper

A list of 65 isolated pairs of galaxies is given in which both components have measured radial velocities and at least one component is a Markarian galaxy. A comparison with a sample of normal pairs indicates that paired Markarian galaxies have a significantly smaller velocity and distance relative to their companion than is true for paired normal galaxies. Markarian galaxies are 50% more luminous and have a higher gas content; and their ratio of orbital mass to luminosity (2.2 + or - 1.6) is typical of late-type galaxies experiencing intensive star formation activity.

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