Intraday Radio Variability in Active Galactic Nuclei
arXiv:astro-ph/9902328 · doi:10.1016/S1387-6473(99)00078-0
Abstract
Rapid flux density variations on timescales of the order of a day or less (Intraday Variability, IDV) in the radio regime are a common phenomenon within the blazar class. Observations with the 100m telescope of the MPIfR showed that the variations occur not only in total intensity, but also in the polarized intensity and in polarization angle. Here we present an overview of our IDV-observations and discuss briefly some models which may explain the effect.
6 pages, 3 figures, needs "elsart" style package. To be published in New Astronomy Reviews, special issue: Proceedings of the 4th EVN/JIVE VLBI Symposium, Eds. Garrett, M.A., Campbell, R.M., & Gurvits, L.J
References in corpus (1)
Cited by in corpus (5)
- Interstellar scintillation as the origin of rapid radio variability in the quasar J1819+3845
- Testing the inverse-Compton catastrophe scenario in the intra-day variable blazar S5 0716+71: II. A search for intra-day variability at millimetre wavelengths with the IRAM 30 m telescope
- The Pearson-Readhead Survey of Compact Extragalactic Radio Sources From Space. II. Analysis of Source Properties
- Space-VLBI Polarimetry of the BL Lac Object S5 0716+714: Rapid Polarization Variability in the VLBI core
- High Resolution Radio Astronomy Using Very Long Baseline Interferometry