Jets in the Fanaroff-Riley class I radio galaxies PKS B1234−723, MRC 1452−517 and PKS B2148−555
We present radio observations made with the Australia Telescope Compact Array to study the jets and lobes of three Fanaroff-Riley class I (FR I) radio galaxies: PKS B1234−723, 1452−517 and B2148−555. The total intensity and polarization radio images of the FR I jets are used to determine jet brightn...
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Veröffentlicht in: | Monthly notices of the Royal Astronomical Society 2002-04, Vol.331 (3), p.717-730 |
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creator | Lloyd, Ben D. Jones, Paul A. |
description | We present radio observations made with the Australia Telescope Compact Array to study the jets and lobes of three Fanaroff-Riley class I (FR I) radio galaxies: PKS B1234−723, 1452−517 and B2148−555. The total intensity and polarization radio images of the FR I jets are used to determine jet brightness and width variations, magnetic field structure and fractional polarization. The equipartition pressure is determined as a function of distance from the galaxies to probe the intergalactic medium. |
doi_str_mv | 10.1046/j.1365-8711.2002.05239.x |
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Not. R. Astron. Soc</addtitle><description>We present radio observations made with the Australia Telescope Compact Array to study the jets and lobes of three Fanaroff-Riley class I (FR I) radio galaxies: PKS B1234−723, 1452−517 and B2148−555. The total intensity and polarization radio images of the FR I jets are used to determine jet brightness and width variations, magnetic field structure and fractional polarization. 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Not. R. Astron. Soc</addtitle><date>2002-04</date><risdate>2002</risdate><volume>331</volume><issue>3</issue><spage>717</spage><epage>730</epage><pages>717-730</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>We present radio observations made with the Australia Telescope Compact Array to study the jets and lobes of three Fanaroff-Riley class I (FR I) radio galaxies: PKS B1234−723, 1452−517 and B2148−555. The total intensity and polarization radio images of the FR I jets are used to determine jet brightness and width variations, magnetic field structure and fractional polarization. The equipartition pressure is determined as a function of distance from the galaxies to probe the intergalactic medium.</abstract><cop>Oxford, UK</cop><pub>Blackwell Science, Ltd</pub><doi>10.1046/j.1365-8711.2002.05239.x</doi><tpages>14</tpages></addata></record> |
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subjects | galaxies: active galaxies: jets intergalactic medium radio continuum: galaxies |
title | Jets in the Fanaroff-Riley class I radio galaxies PKS B1234−723, MRC 1452−517 and PKS B2148−555 |
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