Models of polarized and variable radio emission in the IDV source 0917+624
We examine the power spectrum of intra-day variability and describe the new information which can be derived from wavelet analysis of light curves of the quasar 0917+624. Results for total and polarized flux at 11 cm are shown. Both interstellar scattering and intrinsic models have difficulties in e...
Main Authors: | Beckert, T, Kraus, A, Krichbaum, T, Witzel, A, Zensus, J |
---|---|
Format: | Conference item |
Published: |
2002
|
Similar Items
-
An empirical model for the polarization of pulsar radio emission
by: Melrose, D, et al.
Published: (2005) -
An empirical model for the polarization of pulsar radio emission
by: Melrose, D, et al.
Published: (2006) -
IMAGING AN EVENT HORIZON: MITIGATION OF SOURCE VARIABILITY OF SAGITTARIUS A*
by: Roelofs, Freek, et al.
Published: (2017) -
A high-frequency and multi-epoch VLBI study of 3C 273
by: Krichbaum, T, et al.
Published: (2002) -
THE SOURCE OF COHERENT RADIO-EMISSION IN PULSARS
by: Jones, P
Published: (1980)