Hostname: page-component-77c89778f8-vpsfw Total loading time: 0 Render date: 2024-07-18T06:36:30.607Z Has data issue: false hasContentIssue false

Activity Phenomena Observed at Radio Frequencies in Sprial Galaxies

Published online by Cambridge University Press:  25 May 2016

V.H. Malumian*
Affiliation:
Byurakan Astrophysical Observatory, Byurakan, 378433, Armenia

Abstract

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.

It has been shown that the stage of activity of spiral galaxies depends on both the distance between them and their nearest neighbours and the structure of their central parts.

Type
IV. AGN Related Phenomena
Copyright
Copyright © Astronomical Society of the Pacific 1999 

References

Altschuler, D.R., & Pantoja, C.A. 1984, AJ, 89, 1531 CrossRefGoogle Scholar
Geller, M. & Huchra, J. 1976, ApJS, 32, 409 Google Scholar
Karachentsev, I.D. 1987, Dvojnie Galaktiki (Double Galaxies): Moscow Google Scholar
Malumian, V.H. 1983, Astrofizika, 19, 251 Google Scholar
Malumian, V.H. 1986, Astrofizika, 25, 19 Google Scholar
Malumian, V.H. 1987a, IAU Symposium 121, p.24 Google Scholar
Malumian, V.H. 1987b, Astrofizika, 26, 311 Google Scholar
Malumian, V.H. 1989a, Astrofizika, 30, 223 Google Scholar
Malumian, V.H. 1989b, Astrofizika, 31, 241 Google Scholar
Malumian, V.H. 1990, Astrofizika, 32, 507 Google Scholar
Malumian, V.H. 1996, Astron. Nachr., 317, 101 Google Scholar
Stocke, J.T. 1978, AJ, 83, 348 Google Scholar
Turner, E., & Gott, J.R. 1976, ApJS, 32, 409 Google Scholar
Tovmassian, H.M., & Shakhbazian, E. 1981, Astrofizika, 17, 265 Google Scholar