Bright-rimmed clouds and Young Stellar Objects in IC 1396

dc.contributor.author	Choudhury, R
dc.contributor.author	Bhatt, H. C
dc.date.accessioned	2011-03-17T15:40:17Z
dc.date.available	2011-03-17T15:40:17Z
dc.date.issued	2010
dc.identifier.citation	Ojha, D. K., ed., Interstellar matter and star formation: a multi-wavelength Perspective, An international workshop held as part of the Homi Bhabha Birth Centenary Celebrations, Hyderabad, India Oct 5-7, 2009, pp. 225-227	en
dc.identifier.isbn	978-81-8465-441-7
dc.identifier.uri	http://hdl.handle.net/2248/5426
dc.description	Restricted Access	en
dc.description.abstract	Spectroscopic observations of Young Stellar Objects (YSOs) in IC 1396 are presented. It is found that there is a systematic variation, as a function of position, in W). (Ha) of the YSOs in/around SFO 38 e.g YSOs close to bright-rim have stronger Ha emission and show significant variations compared to the W). CHa) obtained from literature. The nearly coplanar geometry ofHD 206267 and the globules is also discussed using 1.4 GHz images from NRAO VLA Sky Survey.	en
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.ispartofseries	ASI Conference Series, Vol. 1
dc.rights	© Astronomical Society of India	en
dc.subject	ISM: globules	en
dc.subject	Stars: formation	en
dc.subject	Pre-main-sequence	en
dc.subject	HII regions: IC 1396	en
dc.title	Bright-rimmed clouds and Young Stellar Objects in IC 1396	en
dc.type	Article	en