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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2753
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dc.contributor.authorManoj, P-
dc.contributor.authorMaheswar, G-
dc.contributor.authorBhatt, H. C-
dc.date.accessioned2008-07-21T06:58:12Z-
dc.date.available2008-07-21T06:58:12Z-
dc.date.issued2002-09-
dc.identifier.citationBASI, Vol. 30, No. 3, pp. 657 - 660en
dc.identifier.urihttp://hdl.handle.net/2248/2753-
dc.description.abstractWe study the circumstellar environment around intermediate mass young stars in nearby OB associations of different ages. We find that a significant fraction of stars in these associations ha.ve cool circumstellar dust around them. Very few of these stars show any emission line activity. These are young Vega-like systems with tenuoUB dusty disks made of material left over from a more active pre-main sequence phase.en
dc.format.extent146880 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.subjectYoung Stellar Objectsen
dc.subjectOB Associationsen
dc.titleCircumstellar environment around young stars in nearby OB associationsen
dc.typeArticleen
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