On the Line Profiles of Shell Shaped Bipolar Outflows
Abstract
The authors present preliminary data with reference to the shell model suggested by Barral and Cantò (1981), which gives an explicit description of the velocity field along the shell and allows a simple evaluation of the intensity distribution along the shocked surface.
- Publication:
-
Circumstellar Matter
- Pub Date:
- 1987
- Bibcode:
- 1987IAUS..122...87S