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Circumstellar environment around young stars in nearby OB associations

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dc.contributor.author Manoj, P
dc.contributor.author Maheswar, G
dc.contributor.author Bhatt, H. C
dc.date.accessioned 2008-07-21T06:58:12Z
dc.date.available 2008-07-21T06:58:12Z
dc.date.issued 2002-09
dc.identifier.citation BASI, Vol. 30, No. 3, pp. 657 - 660 en
dc.identifier.uri http://hdl.handle.net/2248/2753
dc.description.abstract We 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.extent 146880 bytes
dc.format.mimetype application/pdf
dc.language.iso en en
dc.publisher Astronomical Society of India en
dc.subject Young Stellar Objects en
dc.subject OB Associations en
dc.title Circumstellar environment around young stars in nearby OB associations en
dc.type Article en


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