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The population of planetary nebulae in the galactic bulge

Published online by Cambridge University Press:  07 August 2017

G. Stasińska ,
A. Acker ,
A. Fresneau ,
J.F. Gameiro ,
J. Köppen ,
B. Stenholm  and
R. Tylenda
G. Stasińska
Affiliation:
DAEC, Observatoire de Paris-Meudon F-92195 Meudon Cedex France
A. Acker
Affiliation:
DAEC, Observatoire de Paris-Meudon F-92195 Meudon Cedex France
A. Fresneau
Affiliation:
DAEC, Observatoire de Paris-Meudon F-92195 Meudon Cedex France
J.F. Gameiro
Affiliation:
DAEC, Observatoire de Paris-Meudon F-92195 Meudon Cedex France
J. Köppen
Affiliation:
DAEC, Observatoire de Paris-Meudon F-92195 Meudon Cedex France
B. Stenholm
Affiliation:
DAEC, Observatoire de Paris-Meudon F-92195 Meudon Cedex France
R. Tylenda
Affiliation:
DAEC, Observatoire de Paris-Meudon F-92195 Meudon Cedex France

Extract

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Planetary nebulae are one of the latest phases of evolution of low- and intermediate mass stars and can be used as probes of stellar populations and overall chemical evolution in galaxies. Bulge planetary nebulae offer the advantage of being a sample of objects at known distance. Therefore, their study is essential.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 492
Copyright
Copyright © Kluwer 

References

Acker, A., Köppen, J., Stenholm, B. Raytchev, B. (1991) A&AS 89, 237.Google Scholar
Stasinska, G., Tylenda, R., Acker, A., Stenholm, B. (1991a) A&A, 247, 173.Google Scholar
Stasinska, G., Fresneau, A., da Silva Gameiro, G. F., Acker, A. (1991b) A&A in press.Google Scholar
Tylenda, R., Stasinska, G., Acker, A., Stenholm, B. (1991) A&A 246, 221.Google Scholar