Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-25T18:01:28.028Z Has data issue: false hasContentIssue false

The Radial Velocities of Galaxies Near NGC 7331

Published online by Cambridge University Press:  14 August 2015

C. R. Lynds*
Affiliation:
Kitt Peak National Observatory, Tucson, Ariz., U.S.A.

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.

Radial velocity determinations for galaxies in the vicinity of NGC 7331, including the members of ‘Stephan's Quintet’, show clearly a superposition of at least two distinct physical systems. One includes NGC 7331, NGC 7320 (a Quintet member), and NGC 7343, while the other - seven or eight times more distant - contains the four remaining ‘Quintet’ constituents and six of the seven optical ‘companions’ of NGC 7331.

Type
Research Article
Copyright
Copyright © Reidel 1972 

References

Burbidge, E. M. and Burbidge, G. R.: 1961, Astrophys. J. 134, 244.Google Scholar
Holmberg, E.: 1969, Arkiv Astron. 5, No. 20.Google Scholar
de Vaucouleurs, G. de Vaucouleurs, A.: 1964, Reference Catalog of Bright Galaxies, University of Texas Press, Austin.Google Scholar