| 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 |