Open problems in modeling the solar and stellar environment.
Abstract
Contents: 1. Basic physical properties of the stellar environment. 2. Instabilities. 3. Accretion disks and collimated flows. 4. The stars. 5. Conclusion.
- Publication:
-
Modeling the Stellar Environment: How and Why?
- Pub Date:
- 1989
- Bibcode:
- 1989mse..proc..119Z
- Keywords:
-
- Stellar Atmospheres;
- Stellar Mass Accretion;
- Stellar Models;
- Accretion Disks;
- Collimation;
- Interstellar Magnetic Fields;
- Magnetohydrodynamic Stability;
- Astrophysics;
- Stellar Atmospheres: Models;
- Circumstellar Shells: Models