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PG3, A field in the Bulge of Our Galaxy: Description of a Galactic Model

Published online by Cambridge University Press:  07 August 2017

Y.K. Ng ,
G. Bertelli ,
C. Chiosi ,
A. Bressan ,
H. Habing  and
R.S. Le Poole
Y.K. Ng
Affiliation:
Leiden Observatory, Leiden, the Netherlands
G. Bertelli
Affiliation:
National Council of Research, Rome, Italy Department of Astronomy, Padua, Italy
C. Chiosi
Affiliation:
Department of Astronomy, Padua, Italy
A. Bressan
Affiliation:
Astronomical Observatory, Padua, Italy
H. Habing
Affiliation:
Leiden Observatory, Leiden, the Netherlands
R.S. Le Poole
Affiliation:
Leiden Observatory, Leiden, the Netherlands

Abstract

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Preliminary results are shown of our study on the metallicities and ages of the stellar populations present in different components along the line of sight to field #3 of the Palomar-Groningen Variable Star Survey (PG3) with synthetic Hertzsprung-Russell Diagrams (HRDs).

Type
Contributed Papers
Information
Symposium - International Astronomical Union , Volume 153: Galactic Bulges , 1993 , pp. 319 - 322
Copyright
Copyright © Kluwer 1993 

References

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