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Related papers: Blazars, Gamma Ray Bursts and Galactic superlumina…

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Bright and fast gamma-ray flares with hard spectra have been recently detected from the blazar 3C 279, with apparent GeV luminosities up to $10^{49}$ erg/s. The source is observed to flicker on timescales of minutes with no comparable…

High Energy Astrophysical Phenomena · Physics 2017-07-26 V. Vittorini , M. Tavani , A. Cavaliere

Many similar phenomena occur in astrophysical systems with spatial and mass scales different by many orders of magnitudes. For examples, collimated outflows are produced from the Sun, proto-stellar systems, gamma-ray bursts, neutron star…

Astrophysics · Physics 2009-11-13 Shuang Nan Zhang

Relativistic jets of active galactic nuclei have been known to exist for 100 years. Blazars with their jet pointing close to our line of sight are some of the most variable and extreme objects in the universe, showing emission from radio to…

High Energy Astrophysical Phenomena · Physics 2020-08-18 Talvikki Hovatta , Elina Lindfors

Quasars with flat radio spectra and one-sided, arc-second scale, ~100 mJy GHz radio jets are found to have similar scale X-ray jets in about 60% of such objects, even in short 5 to 10 ks Chandra observations. Jets emit in the GHz band via…

High Energy Astrophysical Phenomena · Physics 2020-03-04 Daniel A. Schwartz

This paper presents the theoretical basis of the fireball/blast wave model, and some implications of recent results on GRB source models and cosmic-ray production from GRBs. BATSE observations of the prompt gamma-ray luminous phase, and…

Astrophysics · Physics 2007-05-23 C. D. Dermer

I review recent progress in the theory of relativistic jet production, with special emphasis on unifying black hole sources of stellar and supermassive size. Observations of both classes of objects, as well as theoretical considerations,…

Astrophysics · Physics 2009-11-10 David L. Meier

The origin of Galactic cosmic rays (CRs) is unknown even though they have traditionally been connected to supernovae based on energetic arguments. In the past decades, Galactic black holes in X-ray binaries (BHXBs) have been proposed as…

High Energy Astrophysical Phenomena · Physics 2024-10-02 Dimitrios Kantzas , Francesca Calore

We report the discovery of fast variability of gamma-ray flares from blazar OJ 287. This blazar is known to be powered by binary system of supermassive black holes. The observed variability time scale T_var < 3-10 hr is much shorter than…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Andrii Neronov , Ievgen Vovk

Gamma-ray bursts are associated with catastrophic cosmic events. They appear when a new black hole, created after the explosion of a massive star or the merger of two compact stars, quickly accretes the matter around it and ejects a…

High Energy Astrophysical Phenomena · Physics 2013-02-27 Jean-Luc Atteia

Relativistic jets of plasma are a key ingredient of many types of Active Galactic Nuclei (AGN). Today we know that AGNs are powered by the accretion of inter stellar material into the gravitational field of a Super Massive Black Hole and…

High Energy Astrophysical Phenomena · Physics 2017-05-24 Giovanni La Mura , Giovanni Busetto , Stefano Ciroi , Piero Rafanelli , Marco Berton , Enrico Congiu , Valentina Cracco , Michele Frezzato

Blazars are a sub-category of radio-loud active galactic nuclei with relativistic jets pointing towards to the observer. They are well-known for their non-thermal variable emission, which practically extends over the whole electromagnetic…

High Energy Astrophysical Phenomena · Physics 2019-01-28 Stella Boula , Maria Petropoulou , Apostolos Mastichiadis

There are now several types of relativistic flows in astrophysical settings. The foremost examples are jets and disks orbiting spinning black holes, pulsar winds and gamma ray bursts. As discussed at this meeting, these flows exhibit…

Astrophysics · Physics 2007-05-23 R. D. Blandford

Since the seminal work of Penrose (1969) and Blandford & Znajek (1977), it has been realized that black hole spin may be an important energy source in astrophysics. The radio-loud/radio-quiet dichotomy in the AGN population is usually…

High Energy Astrophysical Phenomena · Physics 2009-03-25 L. Brenneman , J. M. Miller , K. Nandra , M. Volonteri , M. Cappi , G. Matt , S. Kitamoto , F. Paerels , M. Mendez , R. Smith , M. Nowak , M. Garcia , M. Watson , M. Weisskopf , Y. Terashima , Y. Ueda

A correlation is presented between the pulse lag and the jet-break time for seven BATSE gamma-ray bursts with known redshifts. This is, to our best knowledge, the first known direct tight correlation between a property of the gamma-ray…

Astrophysics · Physics 2009-11-07 Jay D. Salmonson , Titus J. Galama

Gamma Ray Bursts (GRBs) are the most explosive events after the big bang: their energy output corresponds to a sizeable fraction of a solar mass entirely converted into energy in a few seconds. Although many questions about their…

Astrophysics · Physics 2007-05-23 G. Ghisellini

Long duration Gamma-Ray Bursts (GRBs) originate from the core collapse of massive stars, but the identity of the central engine remains elusive. Previous work has shown that rapidly spinning, strongly magnetized proto-neutron stars…

High Energy Astrophysical Phenomena · Physics 2015-05-20 B. D. Metzger , D. Giannios , T. A. Thompson , N. Bucciantini , E. Quataert

There is an increasing number of observational evidence that very high energy gamma-rays in radio-loud active galactic nuclei are produced in the direct vicinity of a supermassive black hole (SMBH), close to the base of a relativistic jet.…

High Energy Astrophysical Phenomena · Physics 2022-11-30 Piotr Banasinski , Wlodek Bednarek

Blazars are high-energy engines providing us natural laboratories to study particle acceleration, relativistic plasma processes, magnetic field dynamics, black hole physics. Key informations are provided by observations at high-energy (in…

High Energy Astrophysical Phenomena · Physics 2017-08-09 F. Tavecchio

Using long-duration general relativistic magnetohydrodynamic simulations of radiatively inefficient accretion discs, the energy, momentum and mass outflow rates from such systems are estimated. Outflows occur via two fairly distinct modes:…

High Energy Astrophysical Phenomena · Physics 2015-06-16 A. Sadowski , R. Narayan , R. Penna , Y. Zhu

Various aspects of the high-energy emission from relativistic jets associated wi th compact astrophysical systems are reviewed. The main leptonic and hadronic processes responsible for the production of high-energy $\gamma$-rays, very-high…

Astrophysics · Physics 2008-11-26 Amir Levinson
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