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Related papers: Periodic variability and binary black hole systems…

200 papers

We present a general relativistic (GR) model of jet variability in active galactic nuclei due to orbiting blobs in helical motion along a funnel or cone shaped magnetic surface anchored to the accretion disk near the black hole. Considering…

High Energy Astrophysical Phenomena · Physics 2015-05-26 P. Mohan , A. Mangalam

We explore the relation between black hole mass ($M_{\rm BH}$) and the motion of the jet components for a sample of blazars. The Very Long Baseline Array (VLBA) 2cm Survey and its continuation: Monitoring of Jets in active galactic nuclei…

Astrophysics · Physics 2009-11-13 Ming Zhou , Xinwu Cao

Supermassive black holes at the centre of active galactic nuclei power some of the most luminous objects in the Universe. Typically, very long baseline interferometric (VLBI) observations of blazars have revealed only funnel-like…

Context: The $\gamma$-ray blazar PKS 2155-304 has attracted considerable attention because of its extreme TeV variability characteristics during an exceptional flaring period in 2006. Among the observed key findings are (i) a minimum…

High Energy Astrophysical Phenomena · Physics 2015-05-19 Frank M. Rieger , Francesca Volpe

Accreting black holes produce powerful relativistic plasma jets which emit radiation across all observable wavelengths but the details of the initial acceleration and confinement of the jet are uncertain. We apply an innovative new model…

High Energy Astrophysical Phenomena · Physics 2015-09-30 William J. Potter , Garret Cotter

Light curves for more than century optical photometric observations of the blazar OJ 287 reveals strong flares with a quasi-period of about 12 years. For a long time, this period has been interpreted by processes in a binary black hole…

High Energy Astrophysical Phenomena · Physics 2021-03-26 M. S. Butuzova , A. B. Pushkarev

The blazar OJ287 is the most promising (and the only) case for an extragalactic binary black hole system inspiralling under the action of gravitational radiation reaction. At present, though it is not possible to directly observe the binary…

High Energy Astrophysical Phenomena · Physics 2012-08-23 M. J. Valtonen , A. Gopakumar , S. Mikkola , K. Wiik , H. J. Lehto

The kinetic energy of bulk relativistic plasma ejected from the central engine of blazars is converted into nonthermal particle energy in the comoving frame through a process of sweeping up material from the surrounding medium. The…

Astrophysics · Physics 2009-10-31 Charles D. Dermer

We review the main topics in the field of blazar multiwavelength variability as a tool to understand the physics and structure of extragalactic jets and their central engine. We address issues such as the cross-correlation between flux…

High Energy Astrophysical Phenomena · Physics 2024-12-17 Claudia M. Raiteri

We study the production of VHE emission in blazars as a superposition of a steady component from a baryonic jet and a time- dependent contribution from an inner e-e+ beam launched by the black hole. Both primary relativistic electrons and…

High Energy Astrophysical Phenomena · Physics 2015-03-20 Matías M. Reynoso , Gustavo E. Romero , María C. Medina

Periodic quasars have been suggested to host supermassive binary black holes (BBHs) in their centers, and their optical/UV periodicities are interpreted as caused by either the Doppler-boosting (DB) effect of continuum emission from the…

Astrophysics of Galaxies · Physics 2021-04-07 Xiang Ji , Youjun Lu , Junqiang Ge , Changshuo Yan , Zihao Song

The blazar AO 0235+164 is a key source for studying the interplay between multi-wavelength variability in its light curves and changes in the position angles and apparent velocities of its parsec-scale jet components. In this work, we…

High Energy Astrophysical Phenomena · Physics 2025-08-21 Flavio Benevenuto da Silva Junior , Anderson Caproni

Black-hole driven relativistic astrophysical jets, such as blazars and gamma-ray bursts (GRBs), are powerful sources of electromagnetic radiation. Their emission is powered by some energy dissipation and particle acceleration mechanism…

High Energy Astrophysical Phenomena · Physics 2019-01-16 Dimitrios Giannios , Dmitri A. Uzdensky

Variable active galactic nuclei showing periodic light curves have been proposed as massive black hole binary (MBHB) candidates. In such scenarios the periodicity can be due to relativistic Doppler-boosting of the emitted light. This…

High Energy Astrophysical Phenomena · Physics 2021-10-13 Massimo Dotti , Matteo Bonetti , Daniel J. D'Orazio , Zoltan Haiman , Luis C. Ho

We investigate the implications of a massive binary system in the centre of the gamma-ray blazar Mkn~501 and show that the periodical behaviour recently observed in the TeV and X-ray lightcurves may possibly be related to the orbital motion…

Astrophysics · Physics 2007-05-23 F. M. Rieger , K. Mannheim

During the motion of a binary pulsar around the Galactic center, the pulsar and its companion experience a wind of dark-matter particles that can affect the orbital motion through dynamical friction. We show that this effect produces a…

High Energy Astrophysical Phenomena · Physics 2015-12-31 Paolo Pani

A single measurement of linear polarization of a nonthermal source provides direct information about the mean direction and level of ordering of the magnetic field. Monitoring of the polarization in blazars, combined with millimeter-wave…

High Energy Astrophysical Phenomena · Physics 2015-06-23 Alan P. Marscher

Rapid variability of the TeV emission in several blazars implies a central black hole mass $M_{BH}<10^8M_\odot$, appreciably smaller than the values estimated from the $M_{BH}-L_{bulg}$ relation, and Doppler factors for the $\gamma$-ray…

Astrophysics · Physics 2009-04-14 Amir Levinson

Blazars are thought to possess a relativistic jet that is pointing toward the direction of the Earth and the elect of relativistic beaming enhances its apparent brightness. They radiate in all wavebands from the radio to the gamma-ray bands…

High Energy Astrophysical Phenomena · Physics 2015-02-11 Ryosuke Itoh , Yasushi FUkazawa , Yasuyuki T. Tanaka , Makoto Uemura , Koji S. Kawabata , Hiroshi Akitaya , Kenji Kawaguchi , Yuka Kanda

We use a continuous wavelet transform to analyze more than two decades of data for the BL~Lac object OJ~287 acquired as part of the UMRAO variability program. We find clear evidence for a persistent modulation of the total flux and…

Astrophysics · Physics 2009-10-30 Philip A. Hughes , Hugh D. Aller , Margo F. Aller