Modelling the Balmer line profiles in the spectra of symbiotic stars
The Balmer emission lines in the spectra of symbiotic stars are often seen to have a double-peaked morphology when observed at high resolution. In this respect, they bear striking similarities to the Balmer line profiles in the spectra of cataclysmic variables, (Cv's) where their origin is ascr...
| Main Author: | |
|---|---|
| Published: |
University of Central Lancashire
1996
|
| Subjects: | |
| Online Access: | http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.361621 |