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Optical Short-Term Variability in the X-Ray-Selected BL Lac Object IE 0317+186 and the Radio-Selected BL Lac Object ON231

Published online by Cambridge University Press:  07 August 2017

F.Z. Cheng
Affiliation:
Center of Astronomy and Astrophysics, CCAST(World Lab.) Center for Astrophysics, University of Science and Technology of China, Hefei, Anhui, P.R.China
J.F. Lu
Affiliation:
Center for Astrophysics, University of Science and Technology of China, Hefei, Anhui, P.R.China
G.Z. Xie
Affiliation:
Center of Astronomy and Astrophysics, CCAST(World Lab.) Yunnan Observatory, Academia Sinica, Kunming, Yunnan, P.R. China
K.H. Li
Affiliation:
Yunnan Observatory, Academia Sinica, Kunming, Yunnan, P.R. China
Z.L. Li
Affiliation:
Yunnan Observatory, Academia Sinica, Kunming, Yunnan, P.R. China
L.F. Wang
Affiliation:
Center for Astrophysics, University of Science and Technology of China, Hefei, Anhui, P.R.China

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In order to compare X-ray-selected BL Lac objects with radio-selected BL Lac objects, we have carried out optical monitoring of some of these objects for about three years at Yunnan Observatory in China. All observations have been made with a CCD-image system at the f/13.3 Cassegrain focus of the 102-cm RCC telescope. The CCD-image system was developed by Ye et al. in Kitt Peak National Observatory of USA (Ye et al., 1985). The filters used were as follows: B-GG385(2mm)+BG12(1mm)+BG18(1mm), V-GG495(2mm)+BG18(2mm). After observing many times, more complete light curves have obtained for the X-ray-selected BL Lac object IE 0317+186 and the radio-selected BL Lac object ON 231, respectively(Fig 1 and Fig 2). Fig 1 shows that IE 0317+186 has a characteristic timescale of about 4.5hours with an amplitudes of ΔV≃0.65 mag. Fig 2 indicates that a timescale of short-term variability in ON 231 is about 70 min with an amplitudes of ΔB≃0.8 mag.

Type
Part 2: BLR and Variability
Copyright
Copyright © Kluwer 1989 

References

Refferences

Fabian, A.C. and Ress, M.J. 1979 X-Ray Astronomy, eds. Baity, W.A. and Peterson, L. E., (Pergaman Press), P381.Google Scholar
Giommi, P., et al. 1987, Ap.J., 322, 662.Google Scholar
Madejski, G.M., and Schwartz, D.A. 1983, Ap.J., 275, 467.Google Scholar
Weistrop, D., et al. 1985, Ap.J., 292, 614.Google Scholar
Worrall, D.M. 1986, The Proceedings of the Workshop “The Continuum Emission in Active Galactic Nuclei”, January 11–14, 1986, Tucson, Arizona, USA.Google Scholar
Worrall, D.M., et al. 1986, Ap.J., 303, 589.Google Scholar
Ye, B.X., et al. 1985, Acta Astron. Sinica., 2, 175.Google Scholar