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A&A 389, 58-67 (2002)
DOI: 10.1051/0004-6361:20020482
Milli-arcsecond scale rotation measure in the CSS quasars 0548+165 and 1524-136
F. Mantovani1, W. Junor2, R. Ricci1, 3, D. J. Saikia4, C. Salter5 and M. Bondi11 Istituto di Radioastronomia, CNR, via P. Gobetti 101, Bologna, Italy
2 University of New Mexico, Albuquerque, New Mexico 87131, USA
3 Scuola Internazionale Superiore di Studi Avanzati, via Beirut 4, 34014 Trieste, Italy
4 National Centre for Radio Astrophysics, TIFR, Post Bag 3, Ganeshkhind, Pune, 411007, India
5 Arecibo Observatory, HC3 Box 53995, Arecibo, Puerto Rico PR 00612, USA
(Received 18 December 2001 / Accepted 3 March 2002)
Abstract
Two Compact Steep-spectrum Sources (CSSs), 0548+165 and
1524-136, chosen from a list of CSSs with polarization
percentages that decrease with decreasing frequency
and high rotation measure values (
RM>450 rad m
-2)
on arcsecond scales, were observed with the VLBA at 4.9 and
8.4 GHz.
RM values up to
104 rad m
-2 were found in
several regions along the jets in both sources. We suggest that a
thin screen of magneto-ionic material with about 1 kpc thickness is
responsible for these high
RMs. The observed depolarization
may be due to beam depolarization and/or inhomogeneities in the
magnetic field.
Key words: techniques: interferometric -- polarization -- galaxies: individual: 0548+165 -- galaxies: individual: 1524-136
Offprint request: F. Mantovani, fmantovani@ira.bo.cnr.it
SIMBAD Objects
© ESO 2002
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