Title:Spectrometry and Linear Spectropolarimetry of Herbig Be Stars PDS 37 and 
PDS 27

Abstract:
We present the results of spectropolarimetric and spectrometric observations of 
Herbig Be stars PDS 37 and PDS 27 both of which have not been studied in depth. 
Spectropolarimetry is a very powerful technique that can be used to study the 
circumstellar environment of stars and map their emission line regions. A 
change in linear polarisation across H-alpha, with depolaristion across the  
absorption component, is detected for both objects as an indication of a 
flattened region namely a disk surrounding the objects. In addition, the 
spectroscopic analysis shows that all visible lines are in emission. We also 
have discussed the accretion rates of these two objects.