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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/763
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dc.contributor.authorVenkataraman, V-
dc.contributor.authorAnandarao, B. G-
dc.date.accessioned2006-03-14T09:48:04Z-
dc.date.available2006-03-14T09:48:04Z-
dc.date.issued2005-06-
dc.identifier.citationBASI, Vol. 33, No. 2, pp. 141-144en
dc.identifier.urihttp://hdl.handle.net/2248/763-
dc.description.abstractWe report initial results from the near-infrared continuum studies on the massive star forming region IRAS 21413+5442. The colour-colour diagram and colour-magnitude diagram were used to determine the evolutionary stage and type of the central object powering the compact HII region. Distance to the object is estimated from H band flux in combination with published radio continuum fluxesen
dc.format.extent247795 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectstar formationen
dc.subjectcompact HII regionen
dc.subjectinfrared photometryen
dc.subjectIRAS sourcesen
dc.subjectIRAS 21413+5442en
dc.titleA near-infrared photometric study of the massive star forming region IRAS 21413+5442en
dc.typeArticleen
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