Hostname: page-component-745bb68f8f-s22k5 Total loading time: 0 Render date: 2025-01-09T09:29:58.415Z Has data issue: false hasContentIssue false
  • English
  • Français

Morphology of Isolated and Grouped Galaxies

Published online by Cambridge University Press:  04 August 2017

Maret Einasto  and
Jaan Einasto
Maret Einasto
Affiliation:
Tartu Astrophysical Observatory 202444 Toravere, Estonia, U.S.S.R.
Jaan Einasto
Affiliation:
Tartu Astrophysical Observatory 202444 Toravere, Estonia, U.S.S.R.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Most galaxies with UV-continuum avoid clusters of galaxies (Lipovetsky 1986). Until recently, however, it was difficult to compare spatial distribution of galaxies with UV-continuum with galaxies of other morphological types, since the number of galaxies with known distances was too small. Rapid accumulation of complete redshift samples in large areas of sky (Huchra 1985) makes such study now possible.

Type
II. Ultraviolet Excess Galaxies
Information
Symposium - International Astronomical Union , Volume 121: Observational Evidences of Activity of Galaxies , 1987 , pp. 101 - 102
Copyright
Copyright © Reidel 1987 

References

Dressler, A.: 1980, Astrophys. J., 236, 351.CrossRefGoogle Scholar
Einasto, J., Saar, E., Kaasik, A. and Chernin, A.: 1974. Nature, 252, 111.CrossRefGoogle Scholar
Einasto, M. and Einasto, J.: 1986. Preprint.Google Scholar
Faber, S. M. and Lin, D. N. C.: 1983. Astrophys. J., 266, L17.Google Scholar
Huchra, J.: 1985. Redshift compilation (unpublished).Google Scholar
Lipovetsky, V. A.: 1986. .Google Scholar
Postman, M. and Geller, M.: 1984. Astrophys. J. 281, 95.Google Scholar
Vorontsov-Velyaminov, B. A.: 1977. Astron. Astrophys. Suppl., 28, 1.Google Scholar