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_λ (Hα) of the YSOs in/around SFO 38 e.g YSOs close to bright-rim have stronger Hα emission and show significant variations compared to the W_λ (Hα) obtained from literature. The nearly coplanar geometry of HD 206267 and the globules is also discussed using 1.4 GHz images from NRAO VLA Sky Survey.