Emission Measure Distribution and Abundances Measurements During High-T Flares

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dc.creatorNordon, R.
dc.creatorBehar, E.
dc.creatorGuedel, M.
dc.date2005-11-06
dc.date.accessioned2026-07-07T06:44:53Z
dc.date.available2026-07-07T06:44:53Z
dc.descriptionThe RSCVn system Sigma Geminorum was observed by XMM-Newton on April 2001 during a large flare. We model the emission measure distribution (EMD) during the flare and during a quiescence period. In the flare, a two phase behaviour is found in which the cool plasma (kT < 2 keV) is not disturbed while a large hot component, at temperatues of kT > 3 keV emerges. Fundamental limitations on EMD modeling of high temperature plasmas are then discussed, in the context of the Sigma Gem flare.
dc.descriptionTo appear in the proceedings of "The X-ray Universe" 2005 Conference. 6 Pages, 5 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0511159
dc.identifierhttp://arxiv.org/abs/astro-ph/0511159
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/102902
dc.subjectAstrophysics
dc.titleEmission Measure Distribution and Abundances Measurements During High-T Flares
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