Arendt (1989) found several high confidence associations of IR emission (IRAS) with supernova remnants (SNR), and the dust seems to trace the radio synchrotron emission in many cases. Whereas the dust temperature and magnetic field strength associated with young remnants are relatively high, we ...
Search for Very High Energy \(\gamma\) -Rays from the SNR 1006 with the HEGRA CT1 Air Imaging Cherenkov TelescopeThe observation of g\\gamma -rays from SuperNova Remnants (SNRs) allows one to study the acceleration of charged particles ([1,2]) by SuperNova blast waves. The remnant of ...
Also, we present the results of long-term observations of the Cygnus region around Cyg X-3 which are revealed the γ-ray emission from the one of nearby object - γCygni SNR. The results of γCygni SNR observation by SHALON are presented with spectral energy distribution, images and ...
Gamma-raysfromSNRsandCosmicRays.ppt,Gamma-rays from SNRs and cosmic rays V.N.Zirakashvili Outline Acceleration of particles at forward and reverse shocks in SNRs Amplification of magnetic fields Radioactivity and electron acceleration Modeling of DSA in
The Galactic Diffuse Gamma-Ray Spectrum from Cosmic-Ray Proton Interactions - Mori - 1997 () Citation Context ...ffuse Galactic emission and of the shell-type SNR RX J1713.7-3946. The GeV Excess With thes-ray production matrix, ... M Ohishi,M Mori,M Walker - 《Icrr U》 被引量: 112...
Fermi gamma-ray space telescopeSpectrum analysisPower spectraPoint sourcesCanonical formsShapesWe present a detailed investigation of the γ-ray emission in the vicinity of the supernova remnant (SNR) W28 (G6.4–0.1) observed by the Large Area Telescope (LAT) on board the Fermi Gamma-ray Space ...
Introduction G54.4Gamma0.3 is an extended shell-type supernova remnant (SNR) in the Galactic plane. We selected this source as a candidate for the interaction of SNRs with the interstellar medium on the base of an investigation of cool IRAS point sources in the direction of SNRs. We found ...
et al.: Evidence for TeV gamma-ray emission from the shell type SNR RX J1713.7-3946. In: Astronomy and Astrophysics 354 (2000), Februar, S. 57-61Muraishi, H., et al. Evidence for TeV gamma-ray emission from the shell type SNR RX J1713.7-3946. Astron. Astrophys. 354, L57-L61 ...
On the gamma-ray spectra radiated by protons accelerated in SNR shocks near molecular clouds: The case of SNR RX J1713.7-3946 M.A. Malkov 1 , P.H. Diamond 1 and R.Z. Sagdeev 2 Abstract Cosmic rays (CRs) are thought to be accelerated in SNRs. The most favorable sit- uation for ...
SNRG284.3–1.8 is an incomplete radio shell with a nonthermal spectrum which is interacting with molecular clouds and which has been associated with the Vela-like pulsar PSRJ1016–5857. High energy (HE; E>100 MeV) gamma-ray emission has been reported for the AGILE and Fermi-LAT Collaborations...