INVERSE COMPTON AND THOMSON SCATTERING OF THE QUASAR 3C 273 EMISSION BY ELECTRONS OF THE NEAREST KNOT OF ITS KILOPARSEC JET

M. S.  Butuzova

doi:10.1615/RadioPhysicsRadioAstronomy.v3.i3.20

无线电物理和天文学期刊

总编辑: Leonid M. Lytvynenko (open in a new tab)

副总编辑s: Alexandr A. Konovalenko (open in a new tab) Valery M. Shulga (open in a new tab) Alexei A. Kostenko (open in a new tab)

每年出版 4 期

ISSN 打印: 2152-274X

ISSN 在线: 2152-2758

INVERSE COMPTON AND THOMSON SCATTERING OF THE QUASAR 3C 273 EMISSION BY ELECTRONS OF THE NEAREST KNOT OF ITS KILOPARSEC JET

卷 3, 册 3, 2012, pp. 197-204

DOI: 10.1615/RadioPhysicsRadioAstronomy.v3.i3.20

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M. S. Butuzova
Institute of Radio Astronomy, National Academy of Sciences of Ukraine, 4, Chervonopraporna St., Kharkiv, 61002, Ukraine

摘要

The X-ray emission of the nearest to the core 3C 273 kiloparsec jet knot A1 is shown to be produced by the inverse Compton scattering of quasar emission rather than by the Thomson scattering. For the last process, a large quantity of thermal plasma is required at the knot, the fact not confirmed by polarization observations. Conclusion is made that the low-energy cut-off occurs at the power-law spectrum of ultrarelativistic electrons in knot A1.

键词: kiloparsec jet, quasar 3C 273, inverse Compton scattering, X-ray emission

对本文的引用

Butuzova M. S., Search for differences in the velocities and directions of the kiloparsec-scale jets of quasars with and without X-ray emission, Astronomy Reports, 60, 3, 2016. Crossref

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