Hostname: page-component-848d4c4894-nr4z6 Total loading time: 0 Render date: 2024-06-08T13:27:43.493Z Has data issue: false hasContentIssue false
  • English
  • Français

Mv−σ Relation: A Universal Law?

Published online by Cambridge University Press:  25 May 2016

S.R. Zaggia
S.R. Zaggia*
Affiliation:
Dip. di Astronomia, Univ. di Padova, Italy

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.

Globular clusters (GC) of different galaxies are thought to be similar in their intrinsic nature, despite the very different environments in which they reside. This statement is mainly based on the luminosity function of GC that appear to be similar for galaxies structurally very different (Secker and Harris 1993). To support the above conclusion only few other GC parameters have been used: integrated colors and metallicity index (Harris 1991). Now, there is a growing body of GC velocity dispersions of other local group galaxies which can be used to perform a useful comparison. The tool for such a comparison is the correlation between GC total luminosity, Mv, and velocity dispersion, σ, found by Djorgovski (1991). This is one of the best non trivial correlation of GC structural parameters that can give important answers to the problems of the formation and evolution of GCs.

Type
Posters: Observations of Star Clusters
Information
Symposium - International Astronomical Union , Volume 174: Dynamical Evolution of Stars Clusters , 1996 , pp. 345 - 346
Copyright
Copyright © Kluwer 1996 

References

Djorgovski, S., 1991, ASP Conf. Ser., 13, 112 Google Scholar
Dubath, P., Mayor, G., and Meylan, G., 1993a, ASP Conf. Ser., 48, 557 Google Scholar
Dubath, P., Meylan, G., and Mayor, G., 1993b, ApJ, 400, 510 CrossRefGoogle Scholar
Harris, W.E., 1991 ARAA, 29, 543 Google Scholar
Peterson, R.C., 1989, in Dynamics of Dense Stellar Systems, ed. Merrit, D., Cambridge University Press, p.161 Google Scholar
Peterson, R.C., 1993, ASP Conf. Ser., 48, 463 Google Scholar
Peterson, R.C., and Cudworth, K.M., 1994, ApJ, 420, 612 Google Scholar
Peterson, R.C., Rees, R.F., and Cudworth, K.M., 1995, ApJ, 443, 124 Google Scholar
Pryor, C., and Meylan, G., 1993, ASP Conf. Ser., 50, 357 Google Scholar
Secker, J., and Harris, W.E., 1993, ApJ, 105, 1358 CrossRefGoogle Scholar
Stryker, et al., 1985, ApJ, 367, 528 Google Scholar
van den Bergh, S., 1981, A&A Sup. Ser., 46, 79 Google Scholar
Zaggia, S.R., Capaccioli, M., Piotto, G., 1995, A&A, in preparation Google Scholar