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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1561
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dc.contributor.authorVaidya, D. B-
dc.contributor.authorAnandarao, B. G-
dc.date.accessioned2007-05-10T05:27:57Z-
dc.date.available2007-05-10T05:27:57Z-
dc.date.issued1993-
dc.identifier.citationBASI, Vol. 21, pp. 591-593en
dc.identifier.urihttp://hdl.handle.net/2248/1561-
dc.description.abstractWe have evaluated the interstellar extinction curve and the ratio R of the total to the selective extinction using exact computations of extinction efficiencies for various grain models. The computed results are compared with the observations in the star forming region, Orion, where the observed R is approximately 5.2. Grains of sizes larger than the normal seem to fit the observed extinction in these regionsen
dc.format.extent169900 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectInterstellar extinctionen
dc.subjectStar forming regionsen
dc.titleInterstellar grains in the regions of anomalous extinctionen
dc.typeArticleen
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