OJ 287 binary black hole system
Mauri Valtonen, Stefano Ciprini

TL;DR
The paper confirms relativistic precession in the binary black hole system OJ 287 through observed outbursts, validating general relativity at higher orders than previous tests, and provides detailed observational results from 2005 to 2010.
Contribution
This study provides the first direct observational confirmation of relativistic precession in the OJ 287 binary black hole system, supporting general relativity.
Findings
Confirmation of relativistic precession through timing of outbursts
Detection of bremsstrahlung radiation consistent with hot gas
Observation of jet rotation aligning with predictions
Abstract
The light curve of the quasar OJ 287 extends from 1891 up today without major gaps. Here we summarize the results of the 2005 - 2010 observing campaign. The main results are the following: (1) The 2005 October optical outburst came at the expected time, thus confirming the general relativistic precession in the binary black hole system. This result disproved the model of a single black hole system with accretion disk oscillations, as well as several toy models of binaries without relativistic precession. In the latter models the main outburst would have been a year later. (2) The nature of the radiation of the 2005 October outburst was expected to be bremsstrahlung from hot gas at the temperature of K. This was confirmed by combined ground based and ultraviolet observations using the XMM-Newton X-ray telescope. (3) A secondary outburst of the same nature was…
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Taxonomy
TopicsAstrophysical Phenomena and Observations
