4
Conferences
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ICN-UNAM
1482bc95ee34f0461176da21871284c8
3
icrc2007@icrc2007.unam.mx
30th International Cosmic Ray Conference
The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.
True
Merida, Mexico
2007-07-03T08:00:00
2007-07-11T19:00:00
2005-09-26T05:04:53
2024-04-12T17:46:55
Mexico/General
Dr.
IGeof-UNAM
40af9343b8bb9d18708b4f0252d5f53c
91
false
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092 (5A)
1
Poster
Gamma ray emission from PWN interacting with molecular clouds
Dr.
MPI f. Physik, Munich, Germany
a9add29ad6a9525659000743154b4b26
Dr.
MPI f. Physik, Munich, Germany
a9add29ad6a9525659000743154b4b26
Dr.
Division of Experimental Physics, University of Lodz, Poland
00e671165c28f7d1f0a3bce78bde62e3
Merida, Mexico
Regency (Hyatt)
2007-07-06T14:45:00
2007-07-06T14:45:00
In this work we consider the situation in which the pulsar (and its nebula) is formed
inside or close to the high density regions of a molecular cloud. Recent models for
the gamma radiation of pulsar wind nebula try to include not only radiation processes
due to the injected leptons but also processes due to injection of relativistic
hadrons into the nebula. Hadrons accelerated during the lifetime of a pulsar can be
partially captured in dense (10^3-10^5 cm^3), magnetized (10^{-5} 10^{-3} G)
molecular clouds, producing gamma-rays for a relatively long time. We compare the
theoretical predictions with PWN candidates observed by MAGIC and HESS in VHE gamma-rays.
paper
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link
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1
More information about the venue
http://www.icrc2007.unam.mx/
link
http://www.icrc2007.unam.mx/
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