Our distorted view of magnetars: application of the Resonant Cyclotron Scattering model

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dc.creatorRea, N.
dc.creatorZane, S.
dc.creatorLyutikov, M.
dc.creatorTurolla, R.
dc.date2006-08-30
dc.date.accessioned2026-07-07T10:39:55Z
dc.date.available2026-07-07T10:39:55Z
dc.descriptionThe X-ray spectra of the magnetar candidates are customarily fitted with an empirical, two component model: an absorbed blackbody and a power-law. However, the physical interpretation of these two spectral components is rarely discussed. It has been recently proposed that the presence of a hot plasma in the magnetosphere of highly magnetized neutron stars might distort, through efficient resonant cyclotron scattering, the thermal emission from the neutron star surface, resulting in the production of non-thermal spectra. Here we discuss the Resonant Cyclotron Scattering (RCS) model, and present its XSPEC implementation, as well as preliminary results of its application to Anomalous X-ray Pulsars and Soft Gamma-ray Repeaters.
dc.description5 pages, 5 color figures; Astrophysics & Space Science, in press ("Isolated Neutron Stars"; London, UK)
dc.identifierhttps://arxiv.org/abs/astro-ph/0608650
dc.identifierhttp://arxiv.org/abs/astro-ph/0608650
dc.identifierAstrophys.SpaceSci.308:61-65,2007
dc.identifierdoi:10.1007/s10509-007-9306-1
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181199
dc.subjectAstrophysics
dc.titleOur distorted view of magnetars: application of the Resonant Cyclotron Scattering model
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