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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/761
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dc.contributor.authorAnandarao, B. G-
dc.date.accessioned2006-03-14T09:40:17Z-
dc.date.available2006-03-14T09:40:17Z-
dc.date.issued2005-06-
dc.identifier.citationBASI, Vol. 33, No. 2, pp. 125-131en
dc.identifier.urihttp://hdl.handle.net/2248/761-
dc.description.abstractWe have initiated a programme to study near-infrared photometry and spectroscopy of low and high mass star forming regions and young stellar objects using the HgCdTe 256 x 256 array camera/spectrograph at the 1.2 m telescope. We describe here some of the significant results obtained under this programme on (i) a low mass T Tauri type pre-main sequence(PMS) star; (ii) an intermediate mass star forming region; and (iii) two high mass star forming regionsen
dc.format.extent187138 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectStar Formationen
dc.subjectPre-main sequence starsen
dc.subjectMolecular Hydrogenen
dc.subjectAccretion disksen
dc.titleNear-infrared photometric and spectroscopic studies on star forming regionsen
dc.typeArticleen
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