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The Thick Disc Population of the Galaxy

Published online by Cambridge University Press:  07 August 2017

A.C. Robin ,
M. Haywood ,
D.K. Ojha ,
O. Bienaymé  and
M. Crézé
A.C. Robin
Affiliation:
Observatoire de Besançon, BP1615, F-25010 Besançoncedex
M. Haywood
Affiliation:
Observatoire de Besançon, BP1615, F-25010 Besançoncedex
D.K. Ojha
Affiliation:
Observatoire de Besançon, BP1615, F-25010 Besançoncedex
O. Bienaymé
Affiliation:
Observatoire de Besançon, BP1615, F-25010 Besançoncedex
M. Crézé
Affiliation:
Observatoire de Strasbourg, 11 rue de l'Université, F-67000 Strasbourg

Extract

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The availability of photometric and astrometric star counts on large fields well distributed in the Galaxy allows us to measure the characteristics of the thick disc population. We use a total of 19 data sets in UBV towards a dozen directions in order to measure the scale height, scale length, local density and metallicity of the intermediate population.

Type
Poster Papers
Information
Symposium - International Astronomical Union , Volume 164: Stellar Populations , 1995 , pp. 388
Copyright
Copyright © Kluwer 1995 

References

Bienaymé, O., Robin, A.C., Crézé, M., 1987, A&A 180, 94.Google Scholar
Haywood, M., 1994, Thèse de doctorat, Observatoire de Paris Google Scholar
Robin, A.C., Crézé, M., 1986, A & A 157, 71 Google Scholar