Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3752
Title: Raman scattering of the synchrotron self-absorbed radiation in accretion discs
Authors: Krishan, V
Keywords: Accretion disks
Quasars
Raman spectra
Self absorption
Synchrotron radiation
Black holes (astronomy)
Electron plasma
Extragalactic radio sources
Nonthermal radiation
Plasma frequencies
Issue Date: Jan-1988
Publisher: Royal Astronomical Society
Citation: Monthly Notices of Royal Astronomical Society, Vol. 230, No.2, pp. 183 - 187
Abstract: The quasar non-thermal continuum in the radio region can undergo Raman scattering in the accretion disc plasma around the central black hole provided that the frequency and the wave vector matching and the threshold conditions are satisfied. The scattered radiation has a frequency ω0/2 ≡ ωp where ω0 is the frequency of the incident radiation and ωp is the electron plasma frequency. The spectral shape of the scattered radiation is significantly different from that of the incident radiation. It is proposed that the observed spectral shape of the radio radiation may be accounted for by including the effects of Raman scattering.
URI: http://hdl.handle.net/2248/3752
ISSN: 0035-8711
Appears in Collections:IIAP Publications

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