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SUMMARY:HAWC detection of SNR W28
DTSTART;VALUE=DATE-TIME:20261019T100000Z
DTEND;VALUE=DATE-TIME:20261019T101000Z
DTSTAMP;VALUE=DATE-TIME:20261112T103449Z
UID:indico-contribution-2253@events.ncbj.gov.pl
DESCRIPTION:Speakers: Suvendu  Giri (The Henryk Niewodniczański Institute
  of Nuclear Physics Polish Academy of Sciences)\nThe W28 supernova remnant
  is a promising site for studying the acceleration and propagation of Gala
 ctic cosmic rays. Its proximity to dense molecular clouds provides a natur
 al environment for cosmic-ray interactions and γ-ray production. We use d
 ata from the High-Altitude Water Cherenkov (HAWC) Observatory to investiga
 te the very-high-energy (VHE\; >100 GeV) γ-ray emission from the W28 regi
 on. We characterize the morphology of the emission and compare its spatial
  distribution with the surrounding molecular-cloud environment. HAWC detec
 ts significant VHE γ-ray emission from the region\, providing an opportun
 ity to probe the connection between the SNR\, cosmic rays\, and nearby mol
 ecular material. Our analysis aims to constrain the origin and propagation
  of the particles responsible for the observed γ-ray emission.\n\nhttps:/
 /events.ncbj.gov.pl/event/502/contributions/2253/
LOCATION:
URL:https://events.ncbj.gov.pl/event/502/contributions/2253/
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