The XMM-Newton view of the radio-quiet neutron star 1E 1207.4-5209

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dc.creatorDe Luca, A.
dc.creatorMereghetti, S.
dc.creatorCaraveo, P. A.
dc.creatorMignani, R. P.
dc.creatorBecker, W.
dc.creatorBignami, G. F.
dc.date2002-11-06
dc.date2002-11-08
dc.date.accessioned2026-07-07T02:06:02Z
dc.date.available2026-07-07T02:06:02Z
dc.descriptionWe have observed the radio-quiet X-ray pulsar 1E 1207.4-5209 with the high throughput EPIC cameras onboard XMM-Newton. The spectrum of this peculiar source is characterized by two broad absorption features which present significant substructures and show a clear phase-dependence. We believe that these features represent a strong evidence for the presence of a magnetized atmosphere containing heavy elements.
dc.description5 pages, 3 eps figures. To appear in "Radio Pulsars" (ASP Conf. Ser.), eds M. Bailes, D. Nice, & S. Thorsett. Figures have been enlarged
dc.identifierhttps://arxiv.org/abs/astro-ph/0211101
dc.identifierhttp://arxiv.org/abs/astro-ph/0211101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5291
dc.subjectAstrophysics
dc.titleThe XMM-Newton view of the radio-quiet neutron star 1E 1207.4-5209
dc.typetext

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