High-resolution spectroscopy of cool stars
Abstract
I will review main results of high-resolution spectroscopy of cool stars with XMM-Newton and Chandra. Spectroscopic determinations of temperature, density and elemental abundances will be discussed and the results for various classes of stars presented. Specific issues discussed include densities of CTTS, the solar and stellar neon problem, CNO abundances of young and evolved stars and the measurement of flare plasma densities.
- Publication:
-
High Resolution X-ray Spectroscopy: Towards IXO
- Pub Date:
- September 2009
- Bibcode:
- 2009hrxs.confE..38S