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There were predictions that blazar <ASTROBJ>OJ 287</ASTROBJ> should have
faded in late 1997 or early 1998. The observational background for these
predictions is the sudden fade of <ASTROBJ>OJ 287</ASTROBJ> in 1989.
Back then, the radio flux decreased steadily for 4-5 months and then the
brightness dropped also in the optical region suddenly for 2-3 weeks to
all time low values, e.g. V=17.4 mag. The predictions are based on a
binary black hole model, where the companion black hole and its
accretion disk eclipse the emission areas of the primary black hole. We
have made observations of <ASTROBJ>OJ 287</ASTROBJ> during the time of
the predicted fade. The results show that, in the optical, <ASTROBJ>OJ
287</ASTROBJ> starts to fade almost linearly in December 1997 until
mid-February 1998, when it suddenly shows a sharp rise and sharp fade,
and starts to get brighter again. The radio observations show no signs
of variability, but the radio flux has been very low since the 1995
outburst. We also have earlier observations since Fall 1993 to Spring
1998, which show that the local minimum reached in February 1998 was the
lowest since 1995. We have made observations with several telescopes in
the optical (UBVRI) and radio (22 and 37 GHz) bands. We discuss the
various events in the light curves and their implications on the
proposed models, especially the binary black hole model by Lehto &
Valtonen (\cite{lv96}), which was used to make the prediction of the
time of the fade. Based on observations made with the Nordic Optical
Telescope, operated on the island of La Palma jointly by Denmark,
Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del
Roque de los Muchachos of the Instituto de Astrofísica de
Canarias, observations at the Perugia Observatory, Perugia, Italy,
observations at the Observatorio Astronómico Nacional, San Pedro
Mártir, Baja California, México, observations at the
Torino Observatory, Torino, Italy, observations at the Tuorla
Observatory, Piikkiö, Finland, and observations at the
Metsähovi Radio Research Station, Metsähovi, Finland.
OJ 287 and the predicted fade of 1998
H. Pietilä;L. O. Takalo;TOSTI, Gino;E. Benítez;B. Chiattelli;R. L. M.;G. Cox;J. A. de;G. d. Francesco;D. Dultzin Hacyan;P. Heinämäki;S. Katajainen;P. Keinänen;H. Korhonen;J. Kotilainen;M. Lainela;J. Licandro;M. Luciani;K. Nilsson;T. Pursimo;C. M. Raiteri;R. Rekola;A. Sillanpää;G. Sobrito;H. Teräsranta;M. Villata;A. Zurita
1999
Abstract
There were predictions that blazar OJ 287 should have
faded in late 1997 or early 1998. The observational background for these
predictions is the sudden fade of OJ 287 in 1989.
Back then, the radio flux decreased steadily for 4-5 months and then the
brightness dropped also in the optical region suddenly for 2-3 weeks to
all time low values, e.g. V=17.4 mag. The predictions are based on a
binary black hole model, where the companion black hole and its
accretion disk eclipse the emission areas of the primary black hole. We
have made observations of OJ 287 during the time of
the predicted fade. The results show that, in the optical, OJ
287 starts to fade almost linearly in December 1997 until
mid-February 1998, when it suddenly shows a sharp rise and sharp fade,
and starts to get brighter again. The radio observations show no signs
of variability, but the radio flux has been very low since the 1995
outburst. We also have earlier observations since Fall 1993 to Spring
1998, which show that the local minimum reached in February 1998 was the
lowest since 1995. We have made observations with several telescopes in
the optical (UBVRI) and radio (22 and 37 GHz) bands. We discuss the
various events in the light curves and their implications on the
proposed models, especially the binary black hole model by Lehto &
Valtonen (\cite{lv96}), which was used to make the prediction of the
time of the fade. Based on observations made with the Nordic Optical
Telescope, operated on the island of La Palma jointly by Denmark,
Finland, Iceland, Norway, and Sweden, in the Spanish Observatorio del
Roque de los Muchachos of the Instituto de Astrofísica de
Canarias, observations at the Perugia Observatory, Perugia, Italy,
observations at the Observatorio Astronómico Nacional, San Pedro
Mártir, Baja California, México, observations at the
Torino Observatory, Torino, Italy, observations at the Tuorla
Observatory, Piikkiö, Finland, and observations at the
Metsähovi Radio Research Station, Metsähovi, Finland.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11391/998193
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