Models of Polarized and Variable Radio Emission for IDV Source 0917+624
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We examine the power spectra of IDV and show the information, which is to be gained by wavelet analysis of light curves of the quasar 0917+624. Results for total and polarized flux at 11cm are shown. Both interstellar scattering and intrinsic models have difficulties in explaining the 1 day period variations. A theoretical model for the time averaged emission is presented, which provides the basis for the analysis of possible variations.
4 pages, 3 figures, to appear in Proceedings of "Particles and Fields in Radio Galaxies", Oxford, 2000, ASP Conf. Series, eds. R. A. Laing and K. M. Blundell
4 pages, 3 figures, to appear in Proceedings of "Particles and Fields in Radio Galaxies", Oxford, 2000, ASP Conf. Series, eds. R. A. Laing and K. M. Blundell