Search Results - "Bednarek, W."

Refine Results
  1. 1

    Inefficient acceleration of electrons in the shocked wind of the massive star Θ1 Ori C within the Trapezium Cluster by Bednarek, W

    “…ABSTRACT Shocked winds of massive stars in young stellar clusters have been proposed as possible sites in which relativistic particles are accelerated…”
    Get full text
    Journal Article
  2. 2

    For how long are particles accelerated in shells of recurrent novae? by Bednarek, W

    “…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…”
    Get full text
    Journal Article
  3. 3

    High-energy radiation from luminous and magnetized stars by Bednarek, W

    “…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…”
    Get full text
    Journal Article
  4. 4
  5. 5

    Hadronic model for the non-thermal radiation from the binary system AR Scorpii by Bednarek, W

    “…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…”
    Get full text
    Journal Article
  6. 6

    Morphology of TeV Gamma-Ray Emission from the Kiloparsec-scale Jets in Radio Galaxies by Bednarek, W.

    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…”
    Get full text
    Journal Article
  7. 7

    HIGH ENERGY NEUTRINOS PRODUCED IN THE ACCRETION DISKS BY NEUTRONS FROM NUCLEI DISINTEGRATED IN THE AGN JETS by Bednarek, W.

    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…”
    Get full text
    Journal Article
  8. 8

    High-energy neutrinos from fast winds in novae by Bednarek, W, Śmiałkowski, A

    “…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…”
    Get full text
    Journal Article
  9. 9

    Absorption effects in the blazar’s γ-ray spectra due to luminous stars crossing the jet by Bednarek, W, Sitarek, J

    “…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…”
    Get full text
    Journal Article
  10. 10

    On the origin of sub-TeV gamma-ray pulsed emission from rotating neutron stars by Bednarek, W.

    “…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…”
    Get full text
    Journal Article
  11. 11

    A model for the two component γ-ray spectra observed from the γ-ray binaries by Bednarek, W.

    “…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…”
    Get full text
    Journal Article
  12. 12

    Variability of GeV gamma-ray emission in QSO B0218+357 due to microlensing on intermediate size structures by Sitarek, J., Bednarek, W.

    “…Strong gravitational lensing leads to an occurrence of multiple images, with different magnifications, of a lensed source. Those magnifications can in turn be…”
    Get full text
    Journal Article
  13. 13

    γ-ray production in young open clusters: Berk 87, Cyg OB2 and Westerlund 2 by Bednarek, W.

    “…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…”
    Get full text
    Journal Article
  14. 14

    TeV gamma-ray emission initiated by the population or individual millisecond pulsars within globular clusters by Bednarek, W., Sitarek, J., Sobczak, T.

    “…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…”
    Get full text
    Journal Article
  15. 15

    On the variability of the GeV and multi-TeV gamma-ray emission from the Crab nebula by Bednarek, W., Idec, W.

    “…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…”
    Get full text
    Journal Article
  16. 16

    TeV gamma-rays from accreting magnetars in massive binaries by Bednarek, W.

    “…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…”
    Get full text
    Journal Article
  17. 17

    On the possibility of sub-TeV γ-ray emission from Cyg X-3 by Bednarek, W.

    “…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…”
    Get full text
    Journal Article
  18. 18

    Two Blobs in a Jet Model for the γ-Ray Emission in Radio Galaxies by Banasi ski, P., Bednarek, W.

    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…”
    Get full text
    Journal Article
  19. 19

    Inverse Compton e± pair cascade model for the γ-ray production in massive binary LSI +61° 303 by Bednarek, W.

    “…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…”
    Get full text
    Journal Article
  20. 20

    Misaligned TeV γ-ray sources in the vicinity of globular clusters by Bednarek, W., Sobczak, T.

    “…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…”
    Get full text
    Journal Article