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

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dc.creatorBeckert, T.
dc.creatorKraus, A.
dc.creatorKrichbaum, T. P.
dc.creatorWitzel, A.
dc.creatorZensus, J. A.
dc.date2000-11-23
dc.date.accessioned2026-07-07T01:56:39Z
dc.date.available2026-07-07T01:56:39Z
dc.descriptionWe 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.
dc.description4 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
dc.identifierhttps://arxiv.org/abs/astro-ph/0011429
dc.identifierhttp://arxiv.org/abs/astro-ph/0011429
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2079
dc.subjectAstrophysics
dc.titleModels of Polarized and Variable Radio Emission for IDV Source 0917+624
dc.typetext

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