Accretion, fluorescent X-ray emission and flaring magnetic structures in YSOs

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dc.creatorFavata, F.
dc.date2004-12-20
dc.date.accessioned2026-07-07T02:16:23Z
dc.date.available2026-07-07T02:16:23Z
dc.descriptionI 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.
dc.descriptionProceedings 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)
dc.identifierhttps://arxiv.org/abs/astro-ph/0412511
dc.identifierhttp://arxiv.org/abs/astro-ph/0412511
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8766
dc.subjectAstrophysics
dc.titleAccretion, fluorescent X-ray emission and flaring magnetic structures in YSOs
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