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.
