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.

Milli-arcsecond scale rotation measure in the CSS quasars 0548+165 and 1524-136

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.
2002
IRA - Istituto di radioastronomia
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/164307
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