Abstract
We present optical polarimetry of the violently variable BL Lacertae object S5 0716 + 714, obtained over a three year period using the 6 m telescope at the Special Astrophysical Observatory in Russia. The degree of polarization is high and variable throughout the observations. With a minimum time resolution of 1 minute, significant variations on a timescale of 10-15 minutes are observed. The variations are complex and not fully sampled by this data, but they are characterized by large amplitude changes on a timescale of about 1 day superposed on smooth variations with a timescale of about 1 week. Possible periods of 12.5, 2.5, and 0.14 days have been discovered. S5 0716 + 714 is a highly compact radio source with nonthermal emission observed across the electromagnetic spectrum out to gamma rays. The optical polarization variations are consistent with relativistically beamed synchrotron emission viewed at a very small angle to the line of sight.
Original language | English (US) |
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Pages (from-to) | 1542-1561 |
Number of pages | 20 |
Journal | Astronomical Journal |
Volume | 119 |
Issue number | 4 |
DOIs | |
State | Published - Apr 2000 |
Keywords
- BL Lacertae objects: individual (0716 + 714)
- Galaxies: nuclei
- Polarization
- Quasars: general
- Radio emission lines
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science