Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/764
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dc.contributor.authorGanesh, S-
dc.contributor.authorJoshi, U. C-
dc.contributor.authorBaliyan, K. S-
dc.contributor.authorOmont, A-
dc.contributor.authorSimon, G-
dc.date.accessioned2006-03-14T10:03:30Z-
dc.date.available2006-03-14T10:03:30Z-
dc.date.issued2005-06-
dc.identifier.citationBASI, Vol. 33, No. 2, pp. 145-150en
dc.identifier.urihttp://hdl.handle.net/2248/764-
dc.description.abstractThe 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 Observatoryen
dc.format.extent242853 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectThe Galaxy - extinction - galactic structureen
dc.subjectstellar populationsen
dc.titleMultiwavelength study of the inner regions of the Milky Way Galaxyen
dc.typeArticleen
Appears in Collections:BASI Publications

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