Hard X-ray/soft gamma-ray Characteristics of the Persistent Emission from Magnetars

Simple item page
dc.creatorKuiper, L.
dc.creatorHartog, P. R. den
dc.creatorHermsen, W.
dc.date2008-10-27
dc.date.accessioned2026-07-07T10:13:24Z
dc.date.available2026-07-07T10:13:24Z
dc.descriptionIn this paper the current status of high-energy research on the hard X-ray characteristics of the persistent emission from magnetars is reviewed. Focus is put on recent intriguing results for 1RXS J1708-40, from phase resolved spectral analysis over a 2 decades wide energy band (~3-300 keV) combining contemporaneous RXTE, XMM and INTEGRAL data. For 1E 1841-045 and SGR 1806-10 we also present updated results. The perspective for future MAXI observations for this source class is also addressed.
dc.description6 pages, 8 figures, Conference Proc. paper: 3rd International Maxi Workshop, 10-12 June, 2008, Wako, Saitama, Japan
dc.identifierhttps://arxiv.org/abs/0810.4801
dc.identifierhttp://arxiv.org/abs/0810.4801
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/172515
dc.subjectAstrophysics
dc.titleHard X-ray/soft gamma-ray Characteristics of the Persistent Emission from Magnetars
dc.typetext

Files

Collections

arXiv