A Few Things We Do Not Know About the Sun and F-G Stars
Abstract
We do not: know how to make realistic model atmospheres, understand convection, consider variation in microturbulent velocity, understand spectroscopy, have good spectra of the Sun or any star, have energy distributions for the Sun or any star, know how to determine abundances, know the abundances of the Sun or any star, have good atomic and molecular data, identify one half of the lines in solar spectrum.
- Publication:
-
Baltic Astronomy
- Pub Date:
- 2002
- Bibcode:
- 2002BaltA..11..101K
- Keywords:
-
- stars: model atmospheres