Polarimetric observations of the quasar 3C 345

Details Polarimetric observations of the quasar 3C 345 Polarimetric observations of the quasar 3C 345

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.233..503m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 233, July 15, 1988, p. 503-509.

Astronomy and Astrophysics

Astronomy

7

Astronomical Models, Polarimetry, Quasars, Balmer Series, Black Body Radiation, Emission Spectra

Scientific paper

Infrared and optical polarimetric observations of the quasar 3C 345 are presented, which show a decrease in the degree of polarization with frequency previously observed by Smith et al., and interpreted by them as the result of dilution of the polarized flux by a non-polarized thermal component (the "blue bump"). The new data are compared to previous fits of this model to 3C 345, and the validity of the model is discussed.

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