Gamma-ray emission expected from Kepler’s SNR
نویسندگان
چکیده
منابع مشابه
Gamma-Ray Emission from X-Ray Binaries
We summarize the current observational picture regarding high-energy emission from Galactic X-ray binaries, reviewing the results of the Compton Gamma Ray Observatory mission. We speculate on the prospects for the GLAST era.
متن کاملNo evidence yet for hadronic TeV gamma - ray emission from SNR RX J 1713 . 7 − 3946
Recent TeV-scale γ-ray observations with the CANGAROO II telescope have led to the claim that the multi-band spectrum of RX J1713.7−3946 cannot be explained as the composite of a synchrotron and an inverse Compton component emitted by a population of relativistic electrons. It was argued that the spectrum of the high-energy emission is a good match to that predicted by pion decay, thus providin...
متن کاملNo evidence yet for hadronic TeV gamma-ray emission from SNR RX J1713-3946
Recent TeV-scale γ-ray observations with the CANGAROO II telescope have led to the claim that the multi-band spectrum of RX J1713.7-3946 cannot be explained as the composite of a synchrotron and an inverse Compton component emitted by a population of relativistic electrons. It was argued that the spectrum of the high-energy emission is a good match to that predicted by pion decay, thus providin...
متن کاملEvidence for TeV gamma - ray emission from the shell type SNR RX J 1713 . 7 − 3946
We report the results of TeV gamma-ray observations of the shell type SNR RX J1713.7−3946 (G347.3−0.5). The discovery of strong non-thermal X-ray emission from the northwest part of the remnant strongly suggests the existence of electrons with energies up to ∼ 100 TeV in the remnant, making the SNR a good candidate TeV gamma-ray source. We observed RX J1713.7−3946 from May to August 1998 with t...
متن کاملGamma ray emission from SNR RX J1713.7-3946 and the origin of galactic cosmic rays
We calculate the flux of non-thermal radiations from the supernova remnant (SNR) RX J1713.7-3946 in the context of the non-linear theory of particle acceleration at shocks, which allows us to take into account self-consistently the dynamical reaction of the accelerated particles, the generation of magnetic fields in the shock proximity and the dynamical reaction of the magnetic field on the pla...
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ژورنال
عنوان ژورنال: Astrophysics and Space Science
سال: 2007
ISSN: 0004-640X,1572-946X
DOI: 10.1007/s10509-007-9401-3