COMPTEL Observation of GRB941017 with Distinct High-Energy Component

2004 ◽  
Author(s):  
Y. Kaneko
Keyword(s):  
High Energy ◽  
Energy Component ◽  
High Energy Component

scholarly journals Simulation studies of the high-energy component of a future imaging Cherenkov telescope array

2008 ◽  
Author(s):  
S. Funk ◽  
J. A. Hinton ◽  
Felix A. Aharonian ◽  
Werner Hofmann ◽  
Frank Rieger
Keyword(s):  
High Energy ◽  
Simulation Studies ◽  
Energy Component ◽  
Telescope Array ◽  
Cherenkov Telescope ◽  
High Energy Component

scholarly journals Galactic Winds and Magnetic Fields from Spiral Galaxies

1990 ◽  
Vol 140 ◽  
pp. 177-181 ◽  
Author(s):  
H.J. Völk ◽  
D. Breitschwerdt ◽  
J.F. McKenzie
Keyword(s):  
Cosmic Rays ◽  
Magnetic Fields ◽  
Mass Loss ◽  
Magnetic Structure ◽  
Essential Role ◽  
Spiral Galaxies ◽  
High Energy ◽  
Energy Component ◽  
Galactic Winds ◽  
High Energy Component

Concentrating on our own Galaxy we discuss the dynamics of the outer halo, its magnetic structure and the occurrence of a supersonic mass loss in the form of a Galactic wind. The cosmic rays, as the nonthermal high energy component, de facto not influenced by gravity, play an essential role in the wind dynamics.

scholarly journals Searching for an additional high-energy component in Fermi-LAT GRB afterglows

2021 ◽  
Author(s):  
X.-B. He ◽  
P.-H. Thomas Tam ◽  
G.-B. Long ◽  
P. S. Pal ◽  
Z. Yong.
Keyword(s):  
High Energy ◽  
Energy Component ◽  
High Energy Component

scholarly journals NEUTRINO EMISSION FROM HIGH-ENERGY COMPONENT GAMMA-RAY BURSTS

2010 ◽  
Vol 721 (2) ◽  
pp. 1891-1899 ◽  
Author(s):  
Julia K. Becker ◽  
Francis Halzen ◽  
Aongus Ó Murchadha ◽  
Martino Olivo
Keyword(s):  
Gamma Ray ◽  
High Energy ◽  
Gamma Ray Bursts ◽  
Neutrino Emission ◽  
Energy Component ◽  
High Energy Component

scholarly journals Erratum: High energy component of giant octupole resonance in medium and heavy mass nuclei

1981 ◽  
Vol 23 (6) ◽  
pp. 2798-2798
Author(s):  
T. Yamagata ◽  
S. Kishimoto ◽  
K. Yuasa ◽  
K. Iwamoto ◽  
B. Saeki ◽  
...  
Keyword(s):  
High Energy ◽  
Energy Component ◽  
High Energy Component

A high energy component of the intense laser-accelerated proton beams detected by stacked CR-39

2013 ◽  
Vol 50 ◽  
pp. 46-49 ◽  
Author(s):  
Masato Kanasaki ◽  
Atsuto Hattori ◽  
Hironao Sakaki ◽  
Yuji Fukuda ◽  
Akifumi Yogo ◽  
...  
Keyword(s):  
High Energy ◽  
Intense Laser ◽  
Energy Component ◽  
Proton Beams ◽  
High Energy Component

scholarly journals ROSAT X-Ray Observations of the Radio Galaxy 4C46.09

1998 ◽  
Vol 188 ◽  
pp. 447-448
Author(s):  
D.A. Leahy
Keyword(s):  
Spectral Analysis ◽  
Radio Source ◽  
Supernova Remnant ◽  
Radio Galaxy ◽  
High Energy ◽  
Energy Component ◽  
X Ray ◽  
Hardness Ratio ◽  
High Energy Component

4C46.09 is the radio source that shows up as a point-like x-ray source inside the supernova remnant HB9 (Leahy, 1987). Leahy, 1987 found a 0.2-4 keV Einstein IPC flux of approximately 1.5 × 10−12erg cm−2s−1 and a significantly higher hardness ratio than the rest of HB9. Too few counts were available for any spectral analysis. Seward et al, 1991, found 4C46.09 to be a large radio galaxy at redshift 0.195 and distance 1280 Mpc (Ho = 50 km s−1Mpc−1). 4C46.09 is of further interest due to the observation of a high energy component in the spectrum of HB9 observed by GINGA (Yamauchi and Koyama, 1993). Whether this was due to HB9 or to 4C46.09 could not be determined.

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