The geometry of PSR B0031-07

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dc.creatorSmits, R.
dc.creatorMitra, D.
dc.creatorStappers, B.
dc.creatorKuijpers, J.
dc.creatorWeltevrede, P.
dc.creatorJessner, A.
dc.creatorGupta, Y.
dc.date2006-12-22
dc.date.accessioned2026-07-07T07:36:43Z
dc.date.available2026-07-07T07:36:43Z
dc.descriptionHere we present the results from an analysis of a multifrequency simultaneous observation of PSR B0031$-$07. We have constructed a geometrical model, based on an empirical relationship between height and frequency of emission, that reproduces many of the observed characteristics. The model suggests very low emission altitudes for this pulsar of only a few kilometers above the star's surface.
dc.descriptionProceedings of the 363. WE-Heraeus Seminar on: Neutron Stars and Pulsars (Posters and contributed talks) Physikzentrum Bad Honnef, Germany, May.14-19, 2006, eds. W.Becker, H.H.Huang, MPE Report 291, pp.161-164
dc.identifierhttps://arxiv.org/abs/astro-ph/0612684
dc.identifierhttp://arxiv.org/abs/astro-ph/0612684
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/120523
dc.subjectAstrophysics
dc.titleThe geometry of PSR B0031-07
dc.typetext

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