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AGB stars and galactic dynamics

Published online by Cambridge University Press:  25 May 2016

H. Dejonghe  and
K. Van Caelenberg
H. Dejonghe
Affiliation:
Sterrenkundig Observatorium, Ghent University, Krijgslaan 281, B-9000 Gent, Belgium
K. Van Caelenberg
Affiliation:
Sterrenkundig Observatorium, Ghent University, Krijgslaan 281, B-9000 Gent, Belgium

Abstract

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AGB stars, seen as a stellar population, can be used to probe the dynamical state of galaxies. The relevant data are mostly positions and line-of-sight velocities, sometimes together with information on chemical composition and/or age. As of now, dynamical models have been made for OH/IR stars and Planetary Nebulae. Other candidates are C stars, S stars, and Miras. We review the methods used and the results obtained so far, for the Milky Way and for (relatively nearby) extragalactic stellar systems.

Information

Type
Part 6. AGB Stars as a Population of Various Galaxies
Information
Symposium - International Astronomical Union , Volume 191: Asymptotic Giant Branch Stars , 1999 , pp. 500 - 510
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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