Dust reddening of Molonglo quasars

Details Dust reddening of Molonglo quasars Dust reddening of Molonglo quasars

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006newar..50..725d&link_type=abstract

New Astronomy Reviews, Volume 50, Issue 9-10, p. 725-727.

Astronomy and Astrophysics

Astronomy

Scientific paper

Balmer ratios have been measured for a well-selected subsample of high-redshift radio-loud quasars from the very complete Molonglo Quasar Sample. Infrared spectra taken with ISAAC at the VLT were used to measure the broad line fluxes and continuum slopes, which give quantitative measures of reddening, and therefore allow comparisons of dust properties over different populations within the sample.

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