XMM-Newton EPIC observations of Her X-1

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dc.creatorRamsay, G.
dc.creatorZane, S.
dc.creatorJimenez-Garate, M. A.
dc.creatorHerder, J. W. den
dc.creatorHailey, C. J.
dc.date2002-01-31
dc.date.accessioned2026-07-07T02:02:34Z
dc.date.available2026-07-07T02:02:34Z
dc.descriptionWe present spin-resolved X-ray data of the neutron star binary Her X-1. We find evidence that the Iron line at 6.4 keV originates from the same location as the blackbody X-ray component. The line width and energy varies over both the spin period and the 35 day precession period. We also find that the correlation between the soft and hard X-ray light curves varies over the 35 day period.
dc.descriptionTo appear in Proc Symp. 'New Visions of the X-ray universe in the XMM_Newton and Chandra era', 26-30 Nov 2001, ESTEC, Netherland, ESA SP-488
dc.identifierhttps://arxiv.org/abs/astro-ph/0201526
dc.identifierhttp://arxiv.org/abs/astro-ph/0201526
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/4082
dc.subjectAstrophysics
dc.titleXMM-Newton EPIC observations of Her X-1
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