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Observational properties of galaxies in small systems

Published online by Cambridge University Press:  12 April 2016

M. Jõeveer
M. Jõeveer*
Affiliation:
Tartu Observatory, Tartumaa 61602, Estonia

Abstract

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The mean absolute luminosities and diameters of galaxies in double and triple configurations are compared with the same characteristics for single galaxies. Members of optical pairs and triplets are used as the sample of single galaxies. The mean luminosities of galaxies in physical pairs and triplets are found to be the same as for single galaxies. At the same absolute luminosity, single galaxies have larger diameters compared to galaxies in pairs and triplets.

Type
Part 2. Properties of Small Groups
Information
International Astronomical Union Colloquium , Volume 174: Small Galaxy Groups , 2000 , pp. 86 - 89
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Karachentsev, I.D. 1972, Soobshch. Spets. Astrofiz. Obs., 7, 3.Google Scholar
Karachentsev, I.D. 1987, Binary galaxies, Moscow, Nauka.Google Scholar
Karachentsev, I.D. Karachentseva, V.E., Lebedev, V.S. 1989, Izv. Spets. Astrofiz. Obs. 27, 67.Google Scholar
Karachentsev, I.D. 1990, Proc. IAU Coll. No 124, 3.Google Scholar
Karachentseva, V.E., Karachentsev, I.D., Shcherbanovskij, A.L. 1979, Izv. Spets. Astrofiz. Obs., 11, 3.Google Scholar
Karachentseva, V.E., Karachentsev, I.D., Lebedev, V.S. 1988, Izv. Spets. Astrofiz. Obs., 26, 42.Google Scholar
White, S.D.M., Valders, F. 1980, MNRAS, 190, 55.CrossRefGoogle Scholar
Wiren, S., Zheng, J.-Q., Valtonen, M.J., Chemin, A.D. 1996, AJ, 111, 160.Google Scholar