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Issue A&A
Volume 389, Number 1, July I 2002
Page(s) 58 - 67
Section Extragalactic astronomy
DOI http://dx.doi.org/10.1051/0004-6361:20020482



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. Bondi1

1  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 $\approx$ 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

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© ESO 2002


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