X-ray Spectroscopy of Cool Stars

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dc.creatorGuedel, M.
dc.date2006-09-11
dc.date.accessioned2026-07-07T07:23:11Z
dc.date.available2026-07-07T07:23:11Z
dc.descriptionHigh-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.
dc.description10 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/
dc.identifierhttps://arxiv.org/abs/astro-ph/0609281
dc.identifierhttp://arxiv.org/abs/astro-ph/0609281
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/115886
dc.subjectAstrophysics
dc.titleX-ray Spectroscopy of Cool Stars
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