Search Results - "Bednarek, W."
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Inefficient acceleration of electrons in the shocked wind of the massive star Θ1 Ori C within the Trapezium Cluster
Published in Monthly notices of the Royal Astronomical Society (01-01-2024)“…ABSTRACT Shocked winds of massive stars in young stellar clusters have been proposed as possible sites in which relativistic particles are accelerated…”
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For how long are particles accelerated in shells of recurrent novae?
Published in Monthly notices of the Royal Astronomical Society (26-07-2022)“…ABSTRACT Galactic novae are at present a well established class of γ-ray sources. We wonder for how long the mechanism of acceleration of electrons operates in…”
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High-energy radiation from luminous and magnetized stars
Published in Monthly notices of the Royal Astronomical Society (01-11-2021)“…ABSTRACT A part of early-type stars is characterized by strong dipole magnetic field that is modified by the outflow of dense wind from the stellar surface. At…”
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GeV–TeV γ-rays produced by electrons in the kpc-scale jet as a result of Comptonization of the inner jet emission
Published in Monthly notices of the Royal Astronomical Society (11-02-2019)Get full text
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5
Hadronic model for the non-thermal radiation from the binary system AR Scorpii
Published in Monthly notices of the Royal Astronomical Society. Letters (01-05-2018)“…Abstract AR Scorpii is a close binary system containing a rotation powered white dwarf and a low-mass M type companion star. This system shows non-thermal…”
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Morphology of TeV Gamma-Ray Emission from the Kiloparsec-scale Jets in Radio Galaxies
Published in The Astrophysical journal (10-03-2020)“…TeV γ rays are observed from a few nearby radio galaxies whose jets are viewed at relatively large angles toward the observer. This emission can be produced in…”
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HIGH ENERGY NEUTRINOS PRODUCED IN THE ACCRETION DISKS BY NEUTRONS FROM NUCLEI DISINTEGRATED IN THE AGN JETS
Published in The Astrophysical journal (20-12-2016)“…ABSTRACT We investigate the consequences of acceleration of nuclei in jets of active galaxies not far from the surface of an accretion disk. The nuclei can be…”
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High-energy neutrinos from fast winds in novae
Published in Monthly notices of the Royal Astronomical Society (18-02-2022)“…ABSTRACT We discuss a scenario in which TeV neutrinos are produced during explosions of novae. It is argued that hadrons are accelerated to very high energies…”
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Absorption effects in the blazar’s γ-ray spectra due to luminous stars crossing the jet
Published in Monthly notices of the Royal Astronomical Society (01-05-2021)“…ABSTRACT γ-ray emission in active galaxies is likely produced within the inner jet, or in the close vicinity of the supermassive black hole (SMBH) at…”
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On the origin of sub-TeV gamma-ray pulsed emission from rotating neutron stars
Published in Monthly notices of the Royal Astronomical Society (11-08-2012)“…Abstract Intriguing sub-TeV tails in the pulsed γ-ray emission from the Crab pulsar have recently been discovered by the Major Atmospheric Gamma-Ray Imaging…”
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A model for the two component γ-ray spectra observed from the γ-ray binaries
Published in Monthly notices of the Royal Astronomical Society. Letters (21-11-2011)“…ABSTRACT Observations of two well‐known binary systems (LS 5039 and LS I +61 303) with the satellite and Cherenkov telescopes revealed the broad‐band γ‐ray…”
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Variability of GeV gamma-ray emission in QSO B0218+357 due to microlensing on intermediate size structures
Published in Monthly notices of the Royal Astronomical Society (21-06-2016)“…Strong gravitational lensing leads to an occurrence of multiple images, with different magnifications, of a lensed source. Those magnifications can in turn be…”
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γ-ray production in young open clusters: Berk 87, Cyg OB2 and Westerlund 2
Published in Monthly notices of the Royal Astronomical Society (21-11-2007)“…Young open clusters are sites of cosmic ray acceleration as indicated by recent detections of the TeV γ-ray sources in the directions of two open clusters (Cyg…”
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TeV gamma-ray emission initiated by the population or individual millisecond pulsars within globular clusters
Published in Monthly notices of the Royal Astronomical Society (01-05-2016)“…Two energetic millisecond pulsars (MSPs) within globular clusters (GCs), J1823-3021A in NGC 6624 and PSR B1821-24 in M28, have been recently discovered to emit…”
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On the variability of the GeV and multi-TeV gamma-ray emission from the Crab nebula
Published in Monthly notices of the Royal Astronomical Society (01-07-2011)“…Recently, the AGILEγ-ray telescope has reported enhanced γ-ray emission above 100 MeV from the direction of the Crab nebula during a period of a few days. This…”
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TeV gamma-rays from accreting magnetars in massive binaries
Published in Monthly notices of the Royal Astronomical Society (11-08-2009)“…This paper focuses on neutron stars (NS) of the magnetar type inside massive binary systems. We determine the conditions under which the matter from the…”
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On the possibility of sub-TeV γ-ray emission from Cyg X-3
Published in Monthly notices of the Royal Astronomical Society (21-07-2010)“…The compact X-ray binary system Cyg X-3 has been recently discovered as a source of GeV γ-rays by the AGILE and the Fermi satellites. It shows emission…”
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Two Blobs in a Jet Model for the γ-Ray Emission in Radio Galaxies
Published in The Astrophysical journal (10-09-2018)“…In the unified scheme, FR I type radio galaxies are identified with the blazar type active galaxies for which jets are aligned at large angles to the line of…”
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Inverse Compton e± pair cascade model for the γ-ray production in massive binary LSI +61° 303
Published in Monthly notices of the Royal Astronomical Society (01-10-2006)“…We apply an inverse Compton e± pair cascade model for γ-ray production in the massive binary system LSI +61° 303 assuming that electrons are accelerated…”
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Misaligned TeV γ-ray sources in the vicinity of globular clusters
Published in Monthly notices of the Royal Astronomical Society (11-12-2014)“…Globular clusters (GCs) contain huge number of low-mass stars and also large number of millisecond pulsars (MSPs). Due to the number of stars, the stellar and…”
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