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Miras and Galactic Populations

Published online by Cambridge University Press:  12 April 2016

M.O. Mennessier ,
X. Luri ,
F. Figueras  and
J. Torra
M.O. Mennessier
Affiliation:
GRAAL, Univ Montpellier II/CNRS, F-34095, Montpellier
X. Luri
Affiliation:
Departament d’Astronomia i Meteorologia, Univ Barcelona, Espagne
F. Figueras
Affiliation:
Departament d’Astronomia i Meteorologia, Univ Barcelona, Espagne
J. Torra
Affiliation:
Departament d’Astronomia i Meteorologia, Univ Barcelona, Espagne

Abstract

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In order to exploit the imminent HIPPARCOS data we have developed a new Maximum-Likelihood method to determine luminosity calibrations and kinematical properties with as bias-free as possible estimates. In most cases the samples are inhomogeneous, containing stars of several types. The method includes a way to separate the different groups. We applied the method to Mira variables contained in the HIPPARCOS Input Catalogue.

Type
Part 2. Poster Papers
Information
International Astronomical Union Colloquium , Volume 155: Astrophysical Applications of Stellar Pulsation , 1995 , pp. 423 - 424
Copyright
Copyright © Astronomical Society of the Pacific 1995

References

Boughaleb, H. 1994, these Univ. Montpellier IIGoogle Scholar
Jura, M. 1992, ApJS, 79, 105 Google Scholar
Luri, X., Mennessier, M.O., Figueras, F., & Torra, J. 1994, in “New approaches in Classification and Data Analysis”, Springer-Verlag, p.672 Google Scholar