Simulating peculiar X-shaped extragalactic radio sources

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dc.contributor.authorLacatus, D.A.
dc.contributor.authorParaschiv, A.R.
dc.contributor.authorTesileanu, O.
dc.date.accessioned2017-06-06T18:26:04Z
dc.date.available2017-06-06T18:26:04Z
dc.date.issued2012
dc.description.abstractPeculiar morphologies have been observed among extragalactic radio sources, which present important sideways features that are yet to be explained. After obtaining the region in the parameter space for which the intended lateral extensions appear, further 2D simulations using PLUTO code were performed. For some selected sets of parameters the effect of resolution on the simulated morphology, and the effect of a toroidal magnetic field on the propagation of the simulated jet in the stratified medium, were considered.uk_UA
dc.description.sponsorshipWe are grateful to Prof. Dr. E. Barna, Prof. Dr. S. Antohe, Prof. Dr. Al. Jipa and the University of Bucharest for providing financial support. D. A. Lacatus would like to thank the University of Bucharest for the grant funding this research. Further thanks go to the reviewer for constructive corrections and suggestions for the improvement of the content included in this proceeding.uk_UA
dc.identifier.citationSimulating peculiar X-shaped extragalactic radio sources / D.A. Lacatus, A.R. Paraschiv, O. Tesileanu // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 2. — С. 180-183. — Бібліогр.: 8 назв. — англ.uk_UA
dc.identifier.issn2227-1481
dc.identifier.urihttps://nasplib.isofts.kiev.ua/handle/123456789/119396
dc.language.isoenuk_UA
dc.publisherГоловна астрономічна обсерваторія НАН Україниuk_UA
dc.relation.ispartofAdvances in Astronomy and Space Physics
dc.statuspublished earlieruk_UA
dc.titleSimulating peculiar X-shaped extragalactic radio sourcesuk_UA
dc.typeArticleuk_UA

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Advances in Astronomy and Space Physics, 2012, вип. 2