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arxiv: astro-ph/0011429 · v1 · submitted 2000-11-23 · 🌌 astro-ph

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Models of Polarized and Variable Radio Emission for IDV Source 0917+624

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classification 🌌 astro-ph
keywords analysisemissionmodelspolarizedvariationsaveragedbasiscurves
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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.

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