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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2745
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dc.contributor.authorAnandarao, B. G-
dc.date.accessioned2008-07-18T07:09:19Z-
dc.date.available2008-07-18T07:09:19Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 631 - 636en
dc.identifier.urihttp://hdl.handle.net/2248/2745-
dc.description.abstractWe have initiated an observational programme on star formation using the 256 x 256 HgCd'Th Infrared Array Camera.(NICMOS3) at the 1.2 m m telescope in Mt. Abu. The observations, being made in the spectral region 1-2.5 pm, involve broad/narrow ba.n.<J, imaging photometry of selected small molecular clouds and medium resolution spectroscopy (with the grating spectrogra.ph of NICMOS 3) of some bright young stellar objects. We have also developed a medium resolution Fabry-Perot Imaging Spectrometer for mapping of regions of emission in a selected emission line. We report here some of the recent results obtained by our group.en
dc.format.extent251907 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectStars:Formationen
dc.subjectHerbig-Haro Flowsen
dc.subjectNear Infrareden
dc.subjectH2 Emissionen
dc.titleNear-Infrared Investigations of Star Forming Regionsen
dc.typeArticleen
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