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SUMMARY:Gamma ray emission from PWN interacting with molecular clouds
DTSTART;VALUE=DATE-TIME:20070706T194500Z
DTEND;VALUE=DATE-TIME:20070706T194500Z
DTSTAMP;VALUE=DATE-TIME:20260613T214714Z
UID:indico-contribution-91@cern.ch
DESCRIPTION:Speakers: Dr. BARTKO\, Hendrik (MPI f. Physik\, Munich\, Germa
 ny)\nIn this work we consider the situation in which the pulsar (and its n
 ebula) is formed\ninside or close to the high density regions of a molecul
 ar cloud. Recent models for\nthe gamma radiation of pulsar wind nebula try
  to include not only radiation processes\ndue to the injected leptons but 
 also processes due to injection of relativistic\nhadrons into the nebula. 
 Hadrons accelerated during the lifetime of a pulsar can be\npartially capt
 ured in dense (10^3-10^5 cm^3)\, magnetized (10^{-5} 10^{-3} G)\nmolecular
  clouds\, producing  gamma-rays for a relatively long time. We compare the
 \ntheoretical predictions with PWN candidates observed by MAGIC and HESS i
 n VHE gamma-rays.\n\nhttps://indico.nucleares.unam.mx/event/4/session/39/c
 ontribution/91
LOCATION:Merida\, Mexico Regency (Hyatt)
URL:https://indico.nucleares.unam.mx/event/4/session/39/contribution/91
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