• One more explanation of superluminal motion

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    • Keywords


      extragalactic radio sources; superluminal motion; Raman scattering

    • Abstract


      The occurrence of superluminal motion in extragalactic radio sources is believed to be quite common. Among others, the geometrical scattering of radio radiation can also cause superluminal expansion and or motion and halo formation, In this paper, the effectiveness of the stimulated Raman scattering in producing these features is investigated. The scattering medium is a plasma whose position, density and temperature decide the rate and angle of scattering. When the radiation from a stationary and constant source gets scattered from a stationary plasma, a halo is formed around the source. However, the scattering of a rotating radiation beam does produce superluminal motion of the virtual source. It is found that the plasma should have the characteristics of the emission-line regions and the intercloud medium in order to Raman scatter the radiation. Since the scattering is polarization dependent, it is possible to estimate the rotation of the electric vector along the direction of the apparent motion of a radio source.

    • Author Affiliations


      V. Krishan1

      1. Indian Institute of Astrophysics, Bangalore - 560034
    • Dates

  • Journal of Astrophysics and Astronomy | News

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