XMM-Newton observation of the drifting pulsar B0943+10

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dc.creatorZhang, Bing
dc.creatorSanwal, Divas
dc.creatorPavlov, George G.
dc.date2005-03-18
dc.date.accessioned2026-07-07T02:17:15Z
dc.date.available2026-07-07T02:17:15Z
dc.descriptionRadio pulsar subpulse drifting has been interpreted as rotation of sub-beams (sparks) of pair plasma produced by intermittent breakdowns of an inner vacuum gap above the pulsar polar cap. This model also predicts strong thermal X-ray emission from the polar cap caused by inflowing particles created in spark discharges. We have observed the best-studied drifting pulsar B0943+10 with XMM-Newton and detected a point source coincident with the radio pulsar position. Its spectrum could be fitted with a thermal blackbody model, although a power-law model is also acceptable. The thermal fit gives a bolometric luminosity L_bol ~ 5 x 10^{28} erg/s and a surface area A ~ 10^3 (T/3MK)^{-4} m^2, much smaller than the conventional polar cap area, 6 x 10^4 m^2. Such thermal radiation can be interpreted as emitted from footprints of sparks drifting in an inner gap of a height h ~ 0.1 - 0.2 r_pc, where r_pc is the polar cap radius. However, the original vacuum gap model by Ruderman and Sutherland requires some modification to reconcile the X-ray and radio data.
dc.descriptionsubmitted to ApJL
dc.identifierhttps://arxiv.org/abs/astro-ph/0503423
dc.identifierhttp://arxiv.org/abs/astro-ph/0503423
dc.identifierAstrophys.J. 624 (2005) L109-L112
dc.identifierdoi:10.1086/430522
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9107
dc.subjectAstrophysics
dc.titleXMM-Newton observation of the drifting pulsar B0943+10
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