Hostname: page-component-7bb8b95d7b-dvmhs Total loading time: 0 Render date: 2024-09-12T04:13:35.839Z Has data issue: false hasContentIssue false
  • English
  • Français

On The Relation between Radius, Luminosity and Surface Brightness in Elliptical Galaxies

Published online by Cambridge University Press:  04 August 2017

E. Recillas-Cruz  and
A. Serrano
E. Recillas-Cruz
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 70-264, México 04510, D.F., México
A. Serrano
Affiliation:
Instituto de Astronomía, Universidad Nacional Autónoma de México, Apdo. Postal 70-264, México 04510, D.F., México

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.

We have analyzed luminosity profiles of E galaxies in six clusters of galaxies. We have found a relationship between radius, luminosity and surface brightness for galaxies in each of the clusters. Moreover, it seems that there is a dependence of the zero point of the relation with environment. This relationship implies that there is not a universal luminosity profile for elliptical galaxies.

Type
Posters
Information
Symposium - International Astronomical Union , Volume 127: Structure and Dynamics of Elliptical Galaxies , 1987 , pp. 389 - 390
Copyright
Copyright © Reidel 1987 

References

REFERENCES

Recillas-Cruz, E., and Serrano, P.G., A. 1986, preprint.Google Scholar
Strom, K.M., and Strom, S.E. 1978a, Astron. J., 83, 73.CrossRefGoogle Scholar
Strom, S.E., and Strom, K.M. 1978b, Astron. J., 83, 732.CrossRefGoogle Scholar
Strom, K.M., and Strom, S.E. 1978c, Astron. J., 83, 1293.CrossRefGoogle Scholar
Strom, S.E., and Strom, K.M. 1978d, Astron. J., 225, L93.CrossRefGoogle Scholar