
TY  - JOUR
A1  - Mutoh, M. 
A1  - Inoue, M. 
A1  - Kameno, S. 
A1  - Asada, K. 
T1  - Rotation Measure and Opacity Asymmetry in 2134+004
JF  - Publications of the Astronomical Society of Australia
JO  - Publ. Astron. Soc.  Aust.
Y1  - 2003
VL  - 20
IS  - 1
SP  - 144
EP  - 146
KW  - dense matter &#8212; galaxies: jets &#8212; galaxies: magnetic fields &#8212; plasmas &#8212; polarisation
UR  - https://doi.org/10.1071/AS03014 
N2  - Based on the free&#8211;free absorption (FFA) model of gigahertz peaked spectrum (GPS) sources, we explain both Faraday rotation asymmetry and opacity asymmetry consistently between two components of a GPS quasar 2134+004. The FFA model assumes dense plasma around the central core to produce FFA, and the difference of path lengths in the plasma toward each component could cause these asymmetries. The component that is closer to the observer has a shorter path length, and consequently, smaller opacity of FFA and lower Faraday rotation. In a simple case, the ratio of Faraday rotation between two components is a function of the ratio of path length, and is the same as the ratio of opacity. Then these two ratios are shown to be essentially the same by our observations. We could thus distinguish between near-side and far-side components by the asymmetries. 
ER  -

