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Studies of the galactic bulges using the post-theoretical mass method

Published online by Cambridge University Press:  07 August 2017

Doru Marian Suran  and
Nedelia Antonia Popescu
Doru Marian Suran
Affiliation:
Astronomical Institute of Romanian Academy, Str. Cutitul de Argint, No. 5, 75212 Bucharest 28, ROMANIA
Nedelia Antonia Popescu
Affiliation:
Astronomical Institute of Romanian Academy, Str. Cutitul de Argint, No. 5, 75212 Bucharest 28, ROMANIA

Abstract

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The results of a new method, Post Theoretical Mass Method (PTM) are presented in order to investigate radial pulsating stars (RPS) in galaxies. Further implications for stellar and galactic astrophysics are also discussed.

Keywords

radial pulsating starsgalaxies-components
Type
Contributed Papers
Information
Symposium - International Astronomical Union , Volume 153: Galactic Bulges , 1993 , pp. 331 - 332
Copyright
Copyright © Kluwer 1993 

References

Becker, S. A., Iben, I., Tuggle, R.S. 1977, Ap. J., 218, 533;CrossRefGoogle Scholar
Suran, M.D. 1985, Topics in Astronomy and Astrophys., 1, 1;Google Scholar
Suran, M.D. 1992, in Proceedings of ESO/EIPC Workshop on Early Type Galaxies, Marciana Marina (in press).Google Scholar