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Conferences
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ICN-UNAM
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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
484
false
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0
Oral
Search for gamma-ray emission from Unidentified EGRET sources Located in the Cygnus Region with the MAGIC Telescope
Mr.
MPI f. Physik, Munich, Germany
a9add29ad6a9525659000743154b4b26
Mr.
MPI f. Physik, Munich, Germany
a9add29ad6a9525659000743154b4b26
Dr.
Division of Experimental Physics, University of Lodz
00e671165c28f7d1f0a3bce78bde62e3
Mrs.
Institut de Física d'Altes Energies, Barcelona
23f1fc53ab82f276132c117fa490c647
Merida, Mexico
Uxmal + Tulum (Holiday Inn)
2007-07-04T10:30:00
2007-07-04T10:42:00
00:12
Many of the unidentified Egret sources are believed to be young pulsars.
Such young not-identified pulsars should be surrounded by pulsar wind
nebulae which are at present well established TeV gamma-ray sources
(like Vela X, MSH 15-52 and G0.9+0.1). Moreover, other type of
gamma-ray sources are likely, i.e. binary systems, molecular clouds,
supernovae
remnants, massive stars. The Milagro experiment has recently reported
a gamma-ray source above ~12 TeV in the Cygnus region, MGRO J2019+37,
which is spatially coincident with the EGRET sources 3EG J2021+3716 /
3EG J2016+3657.
Here we present the results of a search for gamma-ray emission between about
100 GeV and about 10 TeV with the MAGIC telescope from these sources.
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http://www.icrc2007.unam.mx/
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