The infrared and optical variability of OJ 287

Citation
Jh. Fan et al., The infrared and optical variability of OJ 287, ASTR AST SS, 133(2), 1998, pp. 163-169
Citations number
128
Categorie Soggetti
Space Sciences
Journal title
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES
ISSN journal
03650138 → ACNP
Volume
133
Issue
2
Year of publication
1998
Pages
163 - 169
Database
ISI
SICI code
0365-0138(199812)133:2<163:TIAOVO>2.0.ZU;2-O
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 OJ 287. The new optical data in V-band are in agreement with th e 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 magnit ude V has been obtained from our new observations. The new infrared observa tions presented here indicate that the source was at a high level in the in frared band during the observation period. From the available literature, w e have got that the largest variations for UBVRIJHK bands are respectively: Delta U = 4.(m)72; Delta B = 5.(m)93; Delta V = 5.(m)18; Delta R = 4.(m)45 ; Delta I = 4.(m)07; Delta J = 3.(m)87; Delta H = 3.(m)78; Delta K = 3.(m)5 4. A strong correlation is found between the optical and near-infrared band s when the DCF method is used, which suggests that these two bands have the same emission mechanism.