I present some recent developments on high-energy phenomena in YSOs, concentrating on the new evidence for accretion-induced X-ray emission in YSOs, for Fe 6.4 keV fluorescent emission from the disks of YSOs and for very long magnetic structures responsible for intense X-ray flares, likely connecting the star and the circumstellar disk.
@article{arxiv.astro-ph/0412511,
title = {Accretion, fluorescent X-ray emission and flaring magnetic structures in YSOs},
author = {F. Favata},
journal= {arXiv preprint arXiv:astro-ph/0412511},
year = {2007}
}
Comments
Proceedings of a conference on 'Low-mass stars and brown dwarfs: IMF, accretion and activity' held in Volterra (Italy) in October 2004 (Memorie della Societa` Astronomica Italiana)