3 C 191 revisited - Circumquasar shells and radio jets

Details 3 C 191 revisited - Circumquasar shells and radio jets 3 C 191 revisited - Circumquasar shells and radio jets

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...361..362p&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 361, Oct. 1, 1990, p. 362-366.

Astronomy and Astrophysics

Astronomy

9

Absorption Spectra, Interstellar Matter, Quasars, Radio Jets (Astronomy), Stellar Envelopes, Magnetic Fields, Optical Thickness

Scientific paper

The quasar 3C 191 is reexamined in the light of recent rotation measure (RM) observations by Kronberg et al. (1990) and recent He II emission data, and an updated model for the intrinsic formation of the narrow shell of this object is developed. It is argued that the extraordinarily high rotation measure in the jet of this quasar is produced by an intrinsic absorption line system at z(abs) = 1.9453, which has a thin shell configuration produced as a wind from the quasar central regions sweeps up interstellar in an elliptical host galaxy.

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