The optical polarization properties of quasars
The optical polarization properties of quasars
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DOI：
10.1086/168672
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发表时间：
1990-05
期刊：
影响因子：
--
通讯作者：
C. Impey;S. Tapia
中科院分区：
文献类型：
--
作者：
C. Impey;S. Tapia
Optical polarimetry is presented for 163 radio-selected quasars, including a complete sample of 90 sources stronger than 2 Jy at 5 GHz. Synchrotron components are detected in over 30 percent of these flat spectrum quasars, with an optical polarization threshold of p greater than 3 percent. The fraction of polarized quasars is a strong function of the compactness of the radio emission, as measured on VLBI scales. Including the duty cycle correction, essentially every quasar with S(core) greater than S(ext) at radio wavelengths has a prominent blazar component at optical wavelengths. Virtually all of the radio sources with weak emission lines (or BL Lac objects) are highly polarized. Optical and radio polarization are not correlated, and there is no difference in the alpha(ro) distributions of high- and low-polarization quasars, or sources with strong and weak emission lines. Redshift information is incomplete, but BL Lac objects appear to have lower redshifts than strong-lined quasars. 76 refs.
