X-ray Spectroscopy of Cool Stars
arXiv:astro-ph/0609281
Abstract
High-resolution X-ray spectroscopy has addressed not only various topics in coronal physics of stars, but has also uncovered important features relevant for our understanding of stellar evolution and the stellar environment. I summarize recent progress in coronal X-ray spectroscopy and in particular also discuss new results from studies of X-rays from pre-main sequence stars.
10 pages, 16 figures. Proc. "High Resolution X-Ray Spectroscopy: Towards XEUS and Con-X", MSSL, March 27-28, 2006; on-line publication at http://www.mssl.ucl.ac.uk/~gbr/workshop2/