Search for new supernova remnant shells in the Galactic plane with H.E.S.S.
Language
en
Communication dans un congrès
This item was published in
PoS, PoS, 2015-07-30, The Hague. 2016, vol. ICRC2015, p. 886
English Abstract
Amongst the population of TeV gamma-ray sources detected with the High Energy Stereoscopic System (H.E.S.S.) in the Galactic plane, clearly identified supernova remnant (SNR) shells constitute a small but precious source ...Read more >
Amongst the population of TeV gamma-ray sources detected with the High Energy Stereoscopic System (H.E.S.S.) in the Galactic plane, clearly identified supernova remnant (SNR) shells constitute a small but precious source class. TeV-selected SNRs are prime candidates for sources of efficient cosmic-ray acceleration. In this work, we present new SNR candidates that have been identified in the entire H.E.S.S. phase I data set of the Galactic plane recorded over the past ten years. Identification with a known SNR shell candidate was successful for one new source, HESS J1534-571. In other cases, TeV-only shell candidates are challenging to firmly identify as SNRs due to their lack of detected non-thermal emission in lower energy bands. We will discuss how these objects may present an important link between young and evolved SNRs, since their shell emission may be dominated by hadronic processes.Read less <
English Keywords
cosmic radiation: acceleration
energy: high
galaxy
HESS
supernova
gamma ray: VHE
hadronic
emission
Origin
Hal imported