Multiwavelength study of the inner regions of the Milky Way Galaxy

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DC Field	Value	Language
dc.contributor.author	Ganesh, S	-
dc.contributor.author	Joshi, U. C	-
dc.contributor.author	Baliyan, K. S	-
dc.contributor.author	Omont, A	-
dc.contributor.author	Simon, G	-
dc.date.accessioned	2006-03-14T10:03:30Z	-
dc.date.available	2006-03-14T10:03:30Z	-
dc.date.issued	2005-06	-
dc.identifier.citation	BASI, Vol. 33, No. 2, pp. 145-150	en
dc.identifier.uri	http://hdl.handle.net/2248/764	-
dc.description.abstract	The inner regions of the Milky Way have received a lot of attention in recent years. Multiwavelength observations have been made at varying spatial, temporal and spectral resolutions. We have studied the inner regions of the Milky Way using data from the Infrared Space Observatory at mid infrared wavelengths, DENIS and 2MASS at near infrared wavelengths, etc. In the present contribution, we summarize results obtained from these studies. We discuss in particular the M16 star forming region for which complementary near infrared observations were made using the PRL NICMOS array on the 1.2m telescope at the Mt Abu IR Observatory	en
dc.format.extent	242853 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.subject	The Galaxy - extinction - galactic structure	en
dc.subject	stellar populations	en
dc.title	Multiwavelength study of the inner regions of the Milky Way Galaxy	en
dc.type	Article	en
Appears in Collections:	BASI Publications

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