Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.273l..29d&link_type=abstract
Monthly Notices of the Royal Astronomical Society, Volume 273, Issue 2, pp. L29-L33.
Astronomy and Astrophysics
Astronomy
105
Polarization-Radiation Mechanisms, Nonthermal-Galaxies, Active-Ultraviolet, Galaxies.
Scientific paper
We investigate the nebular contribution to the extended UV continua of three high/intermediate-redshift radio galaxies: PKS 2250-41 (z=0.310), 3C 368 (z=1.132) and 4C 41.17 (z=3.8). Using the measured emission-line fluxes, we show that the nebular continuum emitted by the warm gas contributes as much as 60 per cent of the observed UV continua. The nebular component is likely to be important wherever emission lines of large equivalent width are observed; its presence helps to explain the lower-than-expected UV polarizations measured in many radio galaxies.
Clark Natalie
Dickson Ronnie
Morganti Rafaella
Shaw Malcolm
Tadhunter Clive
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