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SUMMARY:H.E.S.S. observations of the supernova remnant RX J0852.0-4622: sh
 ell-type morphology and spectrum of a widely extended VHE gamma-ray source
DTSTART;VALUE=DATE-TIME:20070706T194500Z
DTEND;VALUE=DATE-TIME:20070706T194500Z
DTSTAMP;VALUE=DATE-TIME:20260721T080304Z
UID:indico-contribution-504@cern.ch
DESCRIPTION:Speakers: Mrs. LEMOINE-GOUMARD\, Marianne (CENBG - CNRS - IN2P
 3)\nThe shell-type supernova remnant RX J0852.0-4622 was detected in 2004 
 and re-observed\nbetween December 2004 and May 2005 with the High Energy S
 tereoscopic System\n(H.E.S.S.)\, an array of four Imaging Cherenkov Telesc
 opes located in Namibia and\ndedicated to the observations of gamma-rays a
 bove 100 GeV. The angular resolution of\n< 0.1° and the large field of vi
 ew of H.E.S.S. (5° diameter) are well adapted to\nstudying the morphology
  of the object in very high energy gamma-rays\, which exhibits\na remarkab
 ly thin shell very similar to the features observed in the radio range and
 \nin X-rays. The spectral analysis of the source from 300 GeV to 20 TeV wi
 ll be\npresented. Finally\, the possible origins of the very high energy g
 amma-ray emission\n(Inverse Compton scattering by electrons or the decay o
 f neutral pions produced by\nproton interactions) will be discussed\, on t
 he basis of morphological and spectral\nfeatures obtained at different wav
 elengths.\n\nhttps://indico.nucleares.unam.mx/event/4/session/39/contribut
 ion/504
LOCATION:Merida\, Mexico Regency (Hyatt)
URL:https://indico.nucleares.unam.mx/event/4/session/39/contribution/504
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