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An Outburst of OJ 287

Published online by Cambridge University Press:  04 August 2017

Sen Kikuchi  and
Makoto Inoue
Sen Kikuchi
Affiliation:
Tokyo Astronomical Observatory, Mitaka, Tokyo 181, Japan
Makoto Inoue
Affiliation:
*Nobeyama Radio Observatory, Nobeyama, Minamisaku, Nagano 384-13, Japan

Abstract

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Optical and radio behaviours of OJ 287 in the recent outburst are presented. The light curve is similar to that in the previous outburst in 1970–1971, although the maximum brightness is about 1 mag fainter. The intraday variations are found in both optical and radio regions. We find no periodicity of time scales less than 0.2 days.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 110: VLBI and Compact Radio Sources , 1984 , pp. 181 - 182
Copyright
Copyright © Reidel 1984 

References

Haarala, S., Korhonen, T., Sillanpaa, A., and Salonen, E. 1983, IAU Circ., NO. 3764.Google Scholar
Hagen-Thorn, V. A. 1980, Astrophys. Space Sci., 73, 263.CrossRefGoogle Scholar
Kikuchi, S., Mikami, Y., Konno, M., and Inoue, M. 1976, Publ. Astron. Soc. Japan, 28, 117.Google Scholar
Vaitaoja, E., Lehto, H., Teericorpi, P., Haarala, T., Korhonen, T., Valtonen, M., Terasranta, H., Salonen, E., Urpo, S., Tiuri, M., and Piirola, V. 1983, TURKU-FTL-R26, Informo No. 62.Google Scholar