The FIP effect on late-type stellar coronae: from dwarfs to giants
We present an analysis of high resolution Chandra spectra of late-type stars. Our sample includes giant stars from the Hetzsprung gap to the ''clump'' phase, active stars that have similar fundamental parameters but which have followed quite different evolutionary paths, and RS CVn binary systems. Using a new technique based on the ratios of
Garcia-Alvarez, D. et al.
Fecha de publicación:
8
2004