Formation of relativistic jets by collapsing stars to black holes

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dc.creatorKryvdyk, V.
dc.date2007-03-12
dc.date.accessioned2026-07-07T11:42:49Z
dc.date.available2026-07-07T11:42:49Z
dc.descriptionFormation of relativistic jets in the magnetosphere of collapsing stars is considered. These jets will be formed in the polar caps of magnetosphere of collapsing star, where the stellar magnetic field increases during the collapse and the charged particles are accelerated. The jets will generate non-thermal radiation. The analysis of dynamics and emission of particles in the stellar magnetosphere under collapse shows that collapsing stars can by powerful sources of relativistic jets.
dc.description8 pages, 3 figures, Accepted for publication in Adv. Space Res
dc.identifierhttps://arxiv.org/abs/astro-ph/0703265
dc.identifierhttp://arxiv.org/abs/astro-ph/0703265
dc.identifierAdv.SpaceRes.42:533-537,2008
dc.identifierdoi:10.1016/j.asr.2007.03.021
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/201020
dc.subjectAstrophysics
dc.titleFormation of relativistic jets by collapsing stars to black holes
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