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A Complete, Multicolour Survey of Absolute Proper Motions in the Anticentre Direction at Intermediate Latitude: Kinematics of the Galaxy's Stellar Populations

Published online by Cambridge University Press:  26 July 2016

D.K. Ojha
Affiliation:
Observatoire de Besançon, BP 1615, F-25010 Besançon Cedex, France
O. Bienaymé
Affiliation:
Observatoire de Besançon, BP 1615, F-25010 Besançon Cedex, France
A.C. Robin
Affiliation:
Observatoire de Besançon, BP 1615, F-25010 Besançon Cedex, France

Abstract

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We present the observational results of UBV photometry and absolute proper motions in the anticentre direction at intermediate latitude (l = 167.5°, b = 47.4°) for an 8.6 square degree field. The sample is complete down to V = 17, and the accuracy of the proper motions is better than per century for stars brighter than V = 16. It is attempted here to make an investigation of the structure and kinematics of the Galaxy from absolute proper motions. Details of the present work can be found elsewhere (Ojha et al. 1993).

Type
Part Nine: Galactic Structure
Copyright
Copyright © Kluwer 1994 

References

Bienaymé, O., Mohan, V., Crézé, M., Considère, S. and Robin, A.C., 1992. Astron. Astrophys., 253, 389.Google Scholar
Ojha, D.K., Bienaymé, O., Robin, A.C. and Mohan, V., 1993. Astron. Astrophys., submitted.Google Scholar