XMM-Newton observations of Soft Gamma-ray Repeaters

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dc.creatorMereghetti, S.
dc.creatorEsposito, P.
dc.creatorTiengo, A.
dc.date2006-08-17
dc.date.accessioned2026-07-07T10:39:48Z
dc.date.available2026-07-07T10:39:48Z
dc.descriptionAll the confirmed Soft Gamma-ray Repeaters have been observed with the EPIC instrument on the XMM-Newton satellite. We review the results obtained in these observations, providing the most accurate spectra on the persistent X-ray emission in the 1-10 keV range for these objects, and discuss them in the context of the magnetar interpretation.
dc.description10 pages, 7 figures, 3 tables - Presented at the conference "Isolated Neutron Stars: from the Surface to the Interior", London, UK, 24-28 April 2006
dc.identifierhttps://arxiv.org/abs/astro-ph/0608364
dc.identifierhttp://arxiv.org/abs/astro-ph/0608364
dc.identifierAstrophys.SpaceSci.308:13-23,2007
dc.identifierdoi:10.1007/s10509-007-9384-0
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181154
dc.subjectAstrophysics
dc.titleXMM-Newton observations of Soft Gamma-ray Repeaters
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