Journal Article

A beaming model for the OJ 287 periodic optical outbursts

M. Villata, C. M. Raiteri, A. Sillanpää and L. O. Takalo

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 293, issue 1, pages L13-L16
Published in print January 1998 | ISSN: 0035-8711
Published online January 1998 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1046/j.1365-8711.1998.01244.x
A beaming model for the OJ 287 periodic optical outbursts

Show Summary Details

Preview

Abstract

An analytical model for the description of the quasi-periodic optical outbursts observed in the blazar OJ 287 is presented. The astrophysical scenario that can account for the observed double-peaked structure of the cyclic outbursts consists of a pair of supermassive black holes (BHs) in a binary system, both of them creating a jet. The two jets are bent by the interaction of their magnetized plasma with the ambient medium. The combination of this bending with a long-term precession of the jet axes gives rise to a time-dependent orientation of the emitting outflows. The quasi-periodic optical outbursts that we observe arise from the relativistic beaming effect when part of the bent jets is directed toward us. The theoretical result is a light curve that, for a given choice of the model parameters, describes very well the observational data taken over more than a century, and predicts the future behaviour. This successful agreement between model and observations may be further evidence for the presence of binary BH systems in the cores of active galactic nuclei (AGNs).

Keywords: galaxies: active; BL Lacertae objects: general; BL Lacertae objects: individual: OJ 287; galaxies: jets; galaxies: nuclei

Journal Article.  0 words. 

Subjects: Astronomy and Astrophysics

Full text: subscription required

How to subscribe Recommend to my Librarian

Users without a subscription are not able to see the full content. Please, subscribe or login to access all content.