The variability and periods in the BL Lac AO 0235+164
Abstract
Variability is one of the extreme observational properties of BL Lacertae objects. AO 0235+164 is a well studied BL Lac through the whole electro-magnetic wavebands, it is violently variable in the optical bands. In the present work, we show its optical R band photometric observations carried out during the period of Nov. 2006 to Dec. 2012 using the Ap6E CCD camera attached to the primary focus of the 70 cm meniscus telescope at Abastumani Observatory, Georgia. It shows a large variation of ΔR = 4.88 mag (14.20 - 19.08 mag) during our monitoring period. When periodicity analysis methods are adopted to its R observations from our Abastumani monitoring programme and those in the literature, the signs of some periods, P 1 = 8.26 yr, P 2 = 0.55 yr, P 3 = 0.85 yr, P 4 = 1.99 yr are found.
- Publication:
-
Extragalactic Jets from Every Angle
- Pub Date:
- March 2015
- DOI:
- 10.1017/S1743921315001921
- Bibcode:
- 2015IAUS..313...81F
- Keywords:
-
- galaxies: BL Lacertae Objects: individual (AO 0235+164): photometry