Confirmation of the 12-year optical outburst cycle in blazar OJ 287.

Bibcode
1996A&A...305L..17S
Sillanpaa, A.; Takalo, L. O.; Pursimo, T.; Lehto, H. J.; Nilsson, K.; Teerikorpi, P.; Heinaemaeki, P.; Kidger, M. R.; de Diego, J. A.; Gonzalez-Perez, J. N.; Rodríguez-Espinosa, J. M.; Mahoney, T.; Boltwood, P.; Dultzin-Hacyan, D.; Benitez, E.; Turner, G. W.; Robertson, J. W.; Honeycut, R. K.; Efimov, Yu. S.; Shakhovskoy, N.; Charles, P. A.; Schramm, K. J.; Borgeest, U.; Linde, J. V.; Weneit, W.; Kuehl, D.; Schramm, T.; Sadun, A.; Grashuis, R.; Heidt, J.; Wagner, S.; Bock, H.; Kuemmel, M.; Heines, A.; Fiorucci, M.; Tosti, G.; Ghisellini, G.; Raiteri, C. M.; Villata, M.; de Francesco, G.; Bosio, S.; Latini, G.
Referencia bibliográfica

Astronomy and Astrophysics, v.305, p.L17

Fecha de publicación:
1
1996
Revista
Astronomy and Astrophysics
Número de autores
42
Número de autores del IAC
1
Número de citas
176
Número de citas referidas
147
Descripción
A large monitoring project, OJ-94, was set up with the aim of monitoring the blazar OJ 287 during the predicted optical outburst (in fall 1994, Sillanpaa et al. 1988) and simultaneously to collect a large data base for a small sample of blazars. Through this campaign we have obtained the best ever obtained optical light curve for any extragalactic object. The most prominent feature in the occurring at the beginning of November. This outburst occurred almost exactly at the predicted time.
Tipo
Con árbitro
Blázares

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