Simulating peculiar X-shaped extragalactic radio sources
Peculiar 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 perform...
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Видавець: | Головна астрономічна обсерваторія НАН України |
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Дата: | 2012 |
Автори: | , , |
Формат: | Стаття |
Мова: | English |
Опубліковано: |
Головна астрономічна обсерваторія НАН України
2012
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Назва видання: | Advances in Astronomy and Space Physics |
Онлайн доступ: | http://dspace.nbuv.gov.ua/handle/123456789/119396 |
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Цитувати: | Simulating 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. |
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irk-123456789-1193962017-06-07T03:02:46Z Simulating peculiar X-shaped extragalactic radio sources Lacatus, D.A. Paraschiv, A.R. Tesileanu, O. Peculiar 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. 2012 Article Simulating 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. 2227-1481 http://dspace.nbuv.gov.ua/handle/123456789/119396 en Advances in Astronomy and Space Physics Головна астрономічна обсерваторія НАН України |
institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
collection |
DSpace DC |
language |
English |
description |
Peculiar 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. |
format |
Article |
author |
Lacatus, D.A. Paraschiv, A.R. Tesileanu, O. |
spellingShingle |
Lacatus, D.A. Paraschiv, A.R. Tesileanu, O. Simulating peculiar X-shaped extragalactic radio sources Advances in Astronomy and Space Physics |
author_facet |
Lacatus, D.A. Paraschiv, A.R. Tesileanu, O. |
author_sort |
Lacatus, D.A. |
title |
Simulating peculiar X-shaped extragalactic radio sources |
title_short |
Simulating peculiar X-shaped extragalactic radio sources |
title_full |
Simulating peculiar X-shaped extragalactic radio sources |
title_fullStr |
Simulating peculiar X-shaped extragalactic radio sources |
title_full_unstemmed |
Simulating peculiar X-shaped extragalactic radio sources |
title_sort |
simulating peculiar x-shaped extragalactic radio sources |
publisher |
Головна астрономічна обсерваторія НАН України |
publishDate |
2012 |
url |
http://dspace.nbuv.gov.ua/handle/123456789/119396 |
citation_txt |
Simulating 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. |
series |
Advances in Astronomy and Space Physics |
work_keys_str_mv |
AT lacatusda simulatingpeculiarxshapedextragalacticradiosources AT paraschivar simulatingpeculiarxshapedextragalacticradiosources AT tesileanuo simulatingpeculiarxshapedextragalacticradiosources |
first_indexed |
2023-10-18T20:34:27Z |
last_indexed |
2023-10-18T20:34:27Z |
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1796150555831173120 |