Hostname: page-component-cd9895bd7-gbm5v Total loading time: 0 Render date: 2024-12-27T13:28:28.035Z Has data issue: false hasContentIssue false
  • English
  • Français

Synthetic photometric indices for Galactic globular clusters

Published online by Cambridge University Press:  07 August 2017

M.L. Malagnini ,
L.E. Pasinetti Fracassini ,
S. Covino  and
A. Buzzoni
M.L. Malagnini
Affiliation:
Dipartimento di Fisica, Universita' degli Studi di Milano, Italy
L.E. Pasinetti Fracassini
Affiliation:
Dipartimento di Astronomia, Universita' degli Studi di Trieste, Italy
S. Covino
Affiliation:
Dipartimento di Astronomia, Universita' degli Studi di Trieste, Italy
A. Buzzoni
Affiliation:
Osservatorio Astronomico di Merate, Milano, Italy

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.

A grid of synthetic spectral energy distributions, representative of old stellar populations, has been used to derive colors in different photometric systems, and to compare the theoretical predictions with observational data for galactic globular clusters.

Type
Contributed Papers
Information
Symposium - International Astronomical Union , Volume 153: Galactic Bulges , 1993 , pp. 343 - 344
Copyright
Copyright © Kluwer 1993 

References

Buzzoni, A., 1989, Astrophys. J. Suppl. Ser., 71, 817 CrossRefGoogle Scholar