A magnitude, colour, and proper-motion probe of the Galaxy at an intermediate galactic latitude

dc.contributor.author	Bienayme, O.
dc.contributor.author	Mohan, V.
dc.contributor.author	Creze, M.
dc.contributor.author	Considere, S.
dc.contributor.author	Robin, A. C.
dc.date.accessioned	2010-01-15T04:36:09Z
dc.date.available	2010-01-15T04:36:09Z
dc.date.issued	1992
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/433
dc.description.abstract	A sample survey is being conducted in UBV photometry and proper motions as part of an investigation of galactic structure and evolution. In the present paper we discuss the observational results in a restricted field (1.78 square degree) at intermediate galactic latitude in the direction of the globular cluster M5. The resulting catalogue includes 1180 stars, it is complete down to B = 18, V = 17.4, and U = 18. The plate material has been obtained at the CERGA Schmidt telescope between 1984 and 1990. Glass copies of the Palomar Observatory Sky Survey (POSS, 1955) have been used as first epoch for proper motions. Plates have been digitized using the MAMA machine at the Observatory de Paris.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	aa253-389
dc.subject	Astronomy, Photometry, Kinematics and dynamics of the Galaxy, Structure of the Galaxy, Stellar content of the Galaxy	en_US
dc.title	A magnitude, colour, and proper-motion probe of the Galaxy at an intermediate galactic latitude	en_US
dc.type	Article	en_US