Hostname: page-component-84b7d79bbc-g7rbq Total loading time: 0 Render date: 2024-07-30T07:23:21.705Z Has data issue: false hasContentIssue false
  • English
  • Français

A color-magnitude diagram in field #3 of the Palomar–Groningen Survey

Published online by Cambridge University Press:  07 August 2017

Y. K. Ng ,
G. Bertelli  and
A. Bressan
Y. K. Ng
Affiliation:
Leiden Observatory, P.O. Box 9513, 2300 RA Leiden, The Netherlands
G. Bertelli
Affiliation:
Padova Observatory, Vicolo Osservatorio 5, 35122 Padova, Italy
A. Bressan
Affiliation:
Padova Observatory, Vicolo Osservatorio 5, 35122 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.

Field #3 of the Palomar–Groningen survey (PG3) is thought to be ideal for the study of stellar evolution in the Galactic Bulge (GB). In this field the work of Plaut (1973) and Wesselink (1987) is extended with the aim of constructing a Color Magnitude Diagram (CMD) for a great many stars. This is done by means of automated photographic photometry.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 462
Copyright
Copyright © Kluwer 

References

Bertelli, G. et al. (1990), Astron. Astrophys. Suppl. Ser. 85, 845.Google Scholar
Chiosi, C. et al. (1988), Astron. Astrophys. 196, 84.Google Scholar
Plaut, L. (1973), Astron. Astrophys. Suppl. Ser., 4, 75.Google Scholar
Wesselink, T. (1987), , .Google Scholar