About: Discovery of gamma-ray emission from the shell-type supernova remnant RCW 86 with H.E.S.S     Goto   Sponge   NotDistinct   Permalink

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  • The shell-type supernova remnant (SNR) RCW 86, possibly associated with the historical supernova SN 185, with its relatively large size (about 40' in diameter) and the presence of non-thermal X-rays is a promising target for gamma-ray observations. The high sensitivity, good angular resolution of a few arc minutes and the large field of view of the High Energy Stereoscopic System (H.E.S.S.) make it ideally suited for the study of the gamma-ray morphology of such extended sources. H.E.S.S. observations have indeed led to the discovery of the SNR RCW 86 in very high energy (VHE; E } 100 GeV) gamma-rays. With 31 hours of observation time, the source is detected with a statistical significance of 8.5 sigma and is significantly more extended than the H.E.S.S. point spread function.
  • The shell-type supernova remnant (SNR) RCW 86, possibly associated with the historical supernova SN 185, with its relatively large size (about 40' in diameter) and the presence of non-thermal X-rays is a promising target for gamma-ray observations. The high sensitivity, good angular resolution of a few arc minutes and the large field of view of the High Energy Stereoscopic System (H.E.S.S.) make it ideally suited for the study of the gamma-ray morphology of such extended sources. H.E.S.S. observations have indeed led to the discovery of the SNR RCW 86 in very high energy (VHE; E } 100 GeV) gamma-rays. With 31 hours of observation time, the source is detected with a statistical significance of 8.5 sigma and is significantly more extended than the H.E.S.S. point spread function. (en)
Title
  • Discovery of gamma-ray emission from the shell-type supernova remnant RCW 86 with H.E.S.S
  • Discovery of gamma-ray emission from the shell-type supernova remnant RCW 86 with H.E.S.S (en)
skos:prefLabel
  • Discovery of gamma-ray emission from the shell-type supernova remnant RCW 86 with H.E.S.S
  • Discovery of gamma-ray emission from the shell-type supernova remnant RCW 86 with H.E.S.S (en)
skos:notation
  • RIV/00216208:11320/09:00206589!RIV10-MSM-11320___
http://linked.open...avai/riv/aktivita
http://linked.open...avai/riv/aktivity
  • P(LC527), Z(MSM0021620859)
http://linked.open...iv/cisloPeriodika
  • 2
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
http://linked.open.../riv/druhVysledku
http://linked.open...iv/duvernostUdaju
http://linked.open...titaPredkladatele
http://linked.open...dnocenehoVysledku
  • 310696
http://linked.open...ai/riv/idVysledku
  • RIV/00216208:11320/09:00206589
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • Discovery; gamma-ray; emission; shell-type; supernova; remnant; S (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...odStatuVydavatele
  • US - Spojené státy americké
http://linked.open...ontrolniKodProRIV
  • [477199BB44AB]
http://linked.open...i/riv/nazevZdroje
  • Astrophysical Journal
http://linked.open...in/vavai/riv/obor
http://linked.open...ichTvurcuVysledku
http://linked.open...cetTvurcuVysledku
http://linked.open...vavai/riv/projekt
http://linked.open...UplatneniVysledku
http://linked.open...v/svazekPeriodika
  • 692
http://linked.open...iv/tvurceVysledku
  • Nedbal, Dalibor
  • Rob, Ladislav
  • Aharonian, Felix
http://linked.open...ain/vavai/riv/wos
  • 000263674700040
http://linked.open...n/vavai/riv/zamer
issn
  • 0004-637X
number of pages
http://localhost/t...ganizacniJednotka
  • 11320
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