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Astronomy Colloquium (2017 Spring Semester)

* Date
Jun 08
* Speaker
Juan Carlos Algaba Marcos (KASI)
* Title
Exploring the variability of the flat spectrum radio source 1633+382
* Abstract
 

 

We present multi-frequency simultaneous VLBI radio observations of the flat spectrum radio quasar 1633+382 (4C 38.41) as part of the interferometric monitoring of gamma-ray bright active galactic nuclei (iMOGABA) program combined with additional observations in radio, optical, X-rays and gamma-rays carried out between the period 2012 March – 2015 August. The monitoring of this source reveals a significant increase in its activity in the radio bands, which correlates with other bands from sub-millimeter to gamma-rays. The epochs of the maxima for the two largest $gamma-$ray flares seem to coincide with the ejection of two respective new VLBI components. The evolution of the flares probes the adiabatic losses in agreement with the shock-in-jet model. Derived synchrotron self absorption magnetic fields, of the order of 0.1~mG, do not seem to dramatically change during the flares, and are much smaller than the estimated equipartition magnetic fields, indicating that the source of the flare may be associated with a particle dominated emitting region. This is consistent with considerations suggesting that this region may be located near but downstream the acceleration and collimation region.
 
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