Suzaku Observation of TeV SNR RX J1713.7-3946
نویسندگان
چکیده
منابع مشابه
Evidence 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 کاملStochastic Electron Acceleration in the TeV SNR RX J1713.7-3946 III: Time-Dependent Acceleration
We discuss the generic characteristics of stochastic particle acceleration by fully developed turbulence in collisionless plasmas and show that resonant interactions of particles with high-speed waves dominate the acceleration process. To produce the relativistic electrons inferred from the broadband spectrum of a few well-observed shell-type TeV supernova remnants (STTSNRs) in the leptonic sce...
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 کاملNonthermal X-radiation of SNR RX J1713.7−3946: The Relations to a Nearby Molecular Cloud
The recent X-ray and CO observations of RX J1713.7−3946 show that a significant fraction of the nonthermal X-ray emission of this unique supernova remnant associates, in one way or another, with a molecular cloud interacting with the west part of the shell. This adds a new puzzle in the origin of X-ray emission which cannot be easily explained within the standard model in accordance of which X-...
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ژورنال
عنوان ژورنال: Progress of Theoretical Physics Supplement
سال: 2007
ISSN: 0375-9687
DOI: 10.1143/ptps.169.157