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The pre-main sequence stellar population in galaxies

Published online by Cambridge University Press:  07 August 2017

H. Zinnecker
H. Zinnecker*
Affiliation:
Inst. Astronomie und Astrophysik Universität Würzburg, Germany

Extract

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A complete census of the stellar populations in galaxies must include not only the Main Sequence and various post-Main Sequence populations (SGB, RGB, AGB, HB, plus degenerate objects such as WD and NS) but also the pre-Main Sequence (PMS) stellar population.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 149: The Stellar populations of Galaxies , 1992 , pp. 510
Copyright
Copyright © Kluwer 

References

Mazzitelli, and Moretti, 1980, Ap.J. 235, 955.Google Scholar
Palla, and Stahler, 1990, Ap.J. Lett. 360, L43.CrossRefGoogle Scholar
Zinnecker, , McCaughrean, , and Wilking, 1991, Protostars & Planets III.Google Scholar