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 |