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<supportEmail caption="Support">icrc2007@icrc2007.unam.mx</supportEmail>
<title>30th International Cosmic Ray Conference</title>
<description>The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.</description>
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<startDate>2007-07-03T08:00:00</startDate>
<endDate>2007-07-11T19:00:00</endDate>
<creationDate>2005-09-26T05:04:53</creationDate>
<modificationDate>2024-04-12T17:46:55</modificationDate>
<timezone>Mexico/General</timezone>
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 <title>Discovery of TeV Gamma-Ray Emission in the W28 Region from HESS Observations, and Multiwavelength Comparisons</title>
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   <title>Dr.</title>
   <name first="Gavin" middle="" last="Rowell"></name>
   <organization>School of Chemistry and Physics, University of Adelaide</organization>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
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 <startDate>2007-07-06T14:45:00</startDate>
 <endDate>2007-07-06T14:45:00</endDate>
 <abstract>H.E.S.S. observations of the old-age (more than 10000 yrs; about 0.5 deg diameter) composite SNR W28 
reveal TeV emission situated at its northeastern and southern boundaries. The northeastern TeV source is 
in an 
area where W28 is interacting with a dense molecular cloud, containing OH masers, local radio and X-ray 
peaks. The southern TeV sources are found in a region occupied by several HII regions, including the ultra-
compact HII region W28-A2. Our analysis of NANTEN CO data also reveals a dense molecular cloud 
enveloping 
this southern region. Further details concerning H.E.S.S., NANTEN, and other multiwavelength results will 
be 
presented at the conference.</abstract>
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