activity
20032023
most citedA massive binary black-hole system in OJ287 and a test of general relativity

416 citations · 1.6k across the 44 of their papers we have counts for

collaborators

44 papers

astro-ph.HE2023★ 7 cited

On the need of an ultramassive black hole in OJ 287

Mauri J. Valtonen, Staszek Zola, Achamveedu Gopakumar +25

The highly variable blazar OJ~287 is commonly discussed as an example of a binary black hole system. The 130 year long optical light curve is well explained by a model where the ce…

astro-ph.HE2023★ 7 cited

Observational Implications of OJ 287's Predicted 2022 Disk Impact in the Black Hole Binary Model

Mauri J. Valtonen, Lankeswar Dey, Achamveedu Gopakumar +24

We present a summary of the results of the OJ 287 observational campaign, which was carried out during the 2021/2022 observational season. This season is special in the binary mode…

astro-ph.HE2023★ 22 cited

Refining the 2022 OJ 287 impact flare arrival epoch

Mauri J. Valtonen, Staszek Zola, Gopakumar +24

The bright blazar OJ~287 routinely parades high brightness bremsstrahlung flares, which are explained as being a result of a secondary supermassive black hole (SMBH) impacting the…

astro-ph.HE2022★ 3 cited

Refining the prediction for OJ 287 next impact flare arrival epoch

Mauri J. Valtonen, Staszek Zola, A. Gopakumar +23

The bright blazar OJ~287 routinely parades high brightness bremsstrahlung flares which are explained as being a result of a secondary supermassive black hole (SMBH) impacting the a…

astro-ph.GA2022★ 5 cited

Host galaxy magnitude of OJ 287 from its colours at minimum light

Mauri J. Valtonen, Lankeswar Dey, S. Zola +54

OJ 287 is a BL Lacertae type quasar in which the active galactic nucleus (AGN) outshines the host galaxy by an order of magnitude. The only exception to this may be at minimum ligh…

astro-ph.GA2022

The influence of spin in black hole triplets

Ariel Chitan, Aleksandr Mylläri, Mauri Valtonen

Spin can influence the dynamics of the already chaotic black hole triplet system. We follow this problem in two sets of simulations: first, the Agekian-Anosova region (or region D)…