The Near-Stellar Environment of Cool, Evolved Stars
Abstract
The authors discuss relationships between spectral indicators of chromospheric heating, winds and dust for "low" and "intermediate" mass stars evolving up the RGB and AGB, and suggest new observations from infrared to mm wavelengths which are needed. A full discussion of these relations, which are important for theoretical studies of heating and mass-loss processes, is in preparation.
- Publication:
-
Submillimetre Astronomy
- Pub Date:
- 1990
- DOI:
- 10.1007/978-94-015-6850-0_66
- Bibcode:
- 1990ASSL..158..179J
- Keywords:
-
- Cool Stars: Stellar Envelopes;
- Cool Stars: Mass Loss;
- Cool Stars: Stellar Chromospheres;
- Cool Stars: Stellar Winds