Stellar Coronae with \textit{XMM-Newton} RGS. II. X-ray Variability

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dc.creatorAudard, M.
dc.creatorGuedel, M.
dc.creatorBoggende, A. J. den
dc.creatorBrinkman, A. C.
dc.creatorHerder, J. W. den
dc.creatorKaastra, J. S.
dc.creatorMewe, R.
dc.creatorRaassen, A. J. J.
dc.creatorde Vries, C.
dc.creatorBehar, E.
dc.creatorCottam, J.
dc.creatorKahn, S. M.
dc.creatorPaerels, F. B. S.
dc.creatorPeterson, J. M.
dc.creatorRasmussen, A. P.
dc.creatorSako, M.
dc.creatorBranduardi-Raymont, G.
dc.creatorSakelliou, I.
dc.creatorErd, C.
dc.date2000-11-30
dc.date.accessioned2026-07-07T01:56:46Z
dc.date.available2026-07-07T01:56:46Z
dc.descriptionFirst results from high-resolution coronal spectroscopy of flares with the Reflection Grating Spectrometers on board the \textit{XMM-Newton} satellite are reviewed. Rotational modulation in the X-ray light curve of HR 1099 is discussed. Results from time-dependent spectroscopy of flares in the active stars HR 1099, AB Dor, YY Gem are also presented. Variations in the shape of the emission measure distributions, in the abundances and in the average density of the cool plasma are discussed.
dc.descriptionTo appear in Proc. of "X-ray astronomy 2000",(Palermo Sep. 2000), Eds. R. Giacconi, L. Stella, S. Serio, ASP Conf. Series, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0011574
dc.identifierhttp://arxiv.org/abs/astro-ph/0011574
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2121
dc.subjectAstrophysics
dc.titleStellar Coronae with \textit{XMM-Newton} RGS. II. X-ray Variability
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