The radial structure of the galactic disc

dc.contributor.author	Robin, A. C.
dc.contributor.author	Creze, M.
dc.contributor.author	Mohan, V.
dc.date.accessioned	2010-01-14T09:42:42Z
dc.date.available	2010-01-14T09:42:42Z
dc.date.issued	1992
dc.identifier.citation	This article downloded from ADS Free Online Journal	en_US
dc.identifier.uri	http://hdl.handle.net/123456789/432
dc.description.abstract	Three colour photometry on CCD frames in the Special Ares SpA23 provides a deep probe of the galactic disc in a low absorption window towards the anticenter. Magnitudes to better than 10% at V = 25 and B – V colour down to V = 23 have been obtained. These new data, used in combination with lower magnitude photographic data in a wider field, give a strong evidence that the galactic density scale length is rather short (2.5 kpc) and drops abruptly beyond 6 kpc.	en_US
dc.language.iso	en_US	en_US
dc.relation.ispartofseries	aa265-32
dc.subject	Galactic structure, Stellar populations, Galactic disc, Anticenter, Photometry	en_US
dc.title	The radial structure of the galactic disc	en_US
dc.type	Article	en_US