The infrared and optical variability of OJ 287
Abstract
In this paper, the long-term historical optical (UBVRI) and near-infrared (JHK) data are presented with some new observations in the optical (February 1994-January 1995) and near-infrared (November 1995) bands included for BL Lac object OJ287. The new optical data in V-band are in agreement with the results reported by other authors (Sillanpaa et al. 1996a; Arimoto et al. 1997), a close correlation between the color index of B-V and the magnitude V has been obtained from our new observations; The new infrared observations presented here indicate that the source was at a high level in the infrared band during the observation period; From the available literature, we have got that the largest variations for UBVRIJHK bands are respectively: 4.72mag, 5.93mag, 5.18mag, 4.45mag, 4.07mag, 3.87mag, 3.78mag, and 3.54mag. A strong correlation is found between the optical and near-infrared bands when the DCF method is used, which suggests that these two bands have the same emission mechanism.
Cite
@article{arxiv.astro-ph/9809007,
title = {The infrared and optical variability of OJ 287},
author = {J. H. Fan and G. Adam and G. Z. Xie and S. L. Cao and R. G. Lin and Y. P. Qin and Y. Copin and J. M. Bai and X. Zhang and K. H. Li},
journal= {arXiv preprint arXiv:astro-ph/9809007},
year = {2009}
}
Comments
26 pages, 5 figures, aasms4.sty, to be published in A&AS, November 1998, Vol. 132