Results 101 to 110 of about 88,325 (210)
Optical & X-ray Studies of Ultraluminous X-ray Sources [PDF]
Ultraluminous X-ray Sources (ULXs) are point like X-ray sources situated external to the nucleus of their host galaxy, with inferred X-ray luminosities in excess of 10^{39} erg s^{−1} .
Gladstone, Jeanette Claire +1 more
core
Particle escape from supernova remnant shocks: gamma-ray and cosmic-ray signatures
In the context of the supernova remnant (SNR) paradigm for the origin of Galactic cosmic rays (CRs), the escape process of accelerated particles represents a fundamental piece of information to interpret both the observed CR spectrum and the gamma-ray ...
S. Celli
core
The Counterjet Dominates the Production of PeV Photons from Cyg X-3
We study the physical mechanisms underlying the production of orbitally modulated PeV photons from Cyg X-3, recently discovered by the LHAASO collaboration. Our key findings are as follows.
Andrzej A. Zdziarski +2 more
doaj +1 more source
Likely Detection of GeV γ-Ray Emission from Pulsar Wind Nebula G32.64+0.53 with Fermi-LAT
In this study, we report the likely GeV γ -ray emissions originating from the pulsar PSR J1849-0001's pulsar wind nebula (PWN) G32.64+0.53. Our analysis covers approximately 14.7 yr of data from the Fermi Large Area Telescope Pass 8.
Yifan Xiao, Keyao Wu, Jun Fang
doaj +1 more source
A 2.1 yr periodic oscillation of the gamma-ray flux from the blazar PG 1553+113 has previously been tentatively identified in ∼7 yr of data from the Fermi Large Area Telescope.
S. Abdollahi +100 more
doaj +1 more source
The First LHAASO Catalog of Gamma-Ray Sources
We present the first catalog of very-high-energy and ultra-high-energy gamma-ray sources detected by the Large High Altitude Air Shower Observatory. The catalog was compiled using 508 days of data collected by the Water Cherenkov Detector Array from 2021
Zhen Cao +280 more
doaj +1 more source
Two Models for the Orbital Modulation of Gamma Rays in Cyg X-3
We model the currently available γ -ray data on Cyg X-3 from the Fermi Large Area Telescope. Thanks to Cyg X-3’s very strong γ -ray activity during 2018–2021, the data quality has significantly improved.
Anton Dmytriiev +4 more
doaj +1 more source
Gamma ray astronomy with ARGO-YBJ: First observations.
The ARGO-YBJ experiment is the first EAS detector combining a very high mountain altitude (4300 m a.s.l.) to a full coverage detection surface. These features allow ARGO-YBJ to work in the typical energy range of Cherenkov telescopes, with an energy ...
DE VINCENZI, Mario +5 more
core
X-Ray Observations of Unidentified H.E.S.S. Gamma-Ray Sources
In a survey of the inner part of the Galaxy, performed with the H.E.S.S. Instrument (High energy stereoscopic system) in 2004 and 2005, a large number of new unidentified very high energy (VHE) {gamma}-ray sources above an energy of 100 GeV was ...
Funk, S.
core
X-ray and γ-ray beam interstellar communication and implications for SETI. [PDF]
Beveridge L, Bruhaug G.
europepmc +1 more source

