The short-term radio variability of BL Lacertae objects

Details The short-term radio variability of BL Lacertae objects The short-term radio variability of BL Lacertae objects

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982aj.....87..387a&link_type=abstract

Astronomical Journal, vol. 87, Feb. 1982, p. 387-394.

Astronomy and Astrophysics

Astronomy

23

Bl Lacertae Objects, Radiant Flux Density, Radio Astronomy, Radio Emission, Variability, Calibrating, Error Analysis, Optical Polarization, Quasars, Radio Telescopes

Scientific paper

The variability properties of 37 BL Lacertae objects were monitored during a six-month interval at a frequency of 2380 MHz. Contrary to expectations, it was found that 30 of these objects showed no significant variations in this interval, and that, therefore, rapid radio variability is not a characteristic property of this class of objects. It is suggested that since these objects do not differ significantly from the subclass of high-polarization QSO's, they possibly belong to this same subclass.

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