X-ray and radio emission of kiloparsec jets at large redshifts

For some jets of core dominant quasars we assumed that the X-ray emission of the nearest to the core knots is produced by the inverse Compton scattering on the quasar emission whereas the X-ray emission of distant knots is formed by the inverse Compton scattering on the cosmic microwave background a...

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Бібліографічні деталі
Дата:2012
Автор: Mykhailova, M.S.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2012
Назва видання:Advances in Astronomy and Space Physics
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/119152
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:X-ray and radio emission of kiloparsec jets at large redshifts / M.S. Mykhailova // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 49-52. — Бібліогр.: 11 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id irk-123456789-119152
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spelling irk-123456789-1191522017-06-05T03:04:04Z X-ray and radio emission of kiloparsec jets at large redshifts Mykhailova, M.S. For some jets of core dominant quasars we assumed that the X-ray emission of the nearest to the core knots is produced by the inverse Compton scattering on the quasar emission whereas the X-ray emission of distant knots is formed by the inverse Compton scattering on the cosmic microwave background as it takes place for the 3C 273 jet. Competition of the scattered radiation allows to estimate the luminosity of quasars and the angle between the jet and the line of sight. This angle for a jet of the quasar 1745+624 is 24° ÷ 34°. We found that the ratio of X-ray to radio flux densities conforms to the expected dependence on redshift for the knots of PKS 1127-14 and 1745+624 jets. 2012 Article X-ray and radio emission of kiloparsec jets at large redshifts / M.S. Mykhailova // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 49-52. — Бібліогр.: 11 назв. — англ. 2227-1481 http://dspace.nbuv.gov.ua/handle/123456789/119152 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 For some jets of core dominant quasars we assumed that the X-ray emission of the nearest to the core knots is produced by the inverse Compton scattering on the quasar emission whereas the X-ray emission of distant knots is formed by the inverse Compton scattering on the cosmic microwave background as it takes place for the 3C 273 jet. Competition of the scattered radiation allows to estimate the luminosity of quasars and the angle between the jet and the line of sight. This angle for a jet of the quasar 1745+624 is 24° ÷ 34°. We found that the ratio of X-ray to radio flux densities conforms to the expected dependence on redshift for the knots of PKS 1127-14 and 1745+624 jets.
format Article
author Mykhailova, M.S.
spellingShingle Mykhailova, M.S.
X-ray and radio emission of kiloparsec jets at large redshifts
Advances in Astronomy and Space Physics
author_facet Mykhailova, M.S.
author_sort Mykhailova, M.S.
title X-ray and radio emission of kiloparsec jets at large redshifts
title_short X-ray and radio emission of kiloparsec jets at large redshifts
title_full X-ray and radio emission of kiloparsec jets at large redshifts
title_fullStr X-ray and radio emission of kiloparsec jets at large redshifts
title_full_unstemmed X-ray and radio emission of kiloparsec jets at large redshifts
title_sort x-ray and radio emission of kiloparsec jets at large redshifts
publisher Головна астрономічна обсерваторія НАН України
publishDate 2012
url http://dspace.nbuv.gov.ua/handle/123456789/119152
citation_txt X-ray and radio emission of kiloparsec jets at large redshifts / M.S. Mykhailova // Advances in Astronomy and Space Physics. — 2012. — Т. 2., вип. 1. — С. 49-52. — Бібліогр.: 11 назв. — англ.
series Advances in Astronomy and Space Physics
work_keys_str_mv AT mykhailovams xrayandradioemissionofkiloparsecjetsatlargeredshifts
first_indexed 2023-10-18T20:33:52Z
last_indexed 2023-10-18T20:33:52Z
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