4 Conferences false [["minutes", "Minutes"], ["1", "More information about the venue"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]] ICN-UNAM 1482bc95ee34f0461176da21871284c8 3 icrc2007@icrc2007.unam.mx 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 IGeof-UNAM 40af9343b8bb9d18708b4f0252d5f53c 493 false [["minutes", "Minutes"], ["1", "More information about the venue"], ["notes", "Notes"], ["paper", "Paper"], ["poster", "Poster"], ["slides", "Slides"], ["summary", "Summary"]] OG.2.2 0 Oral Max-Planck-Insitut für Kernphysik, Heidelberg 164e9b5f6a7b777ed656ee0126e8b55e Max-Planck-Insitut für Kernphysik, Heidelberg 164e9b5f6a7b777ed656ee0126e8b55e Max-Planck-Insitut für Kernphysik, Heidelberg d41d8cd98f00b204e9800998ecf8427e Institut für Physik, Humboldt-Universität zu Berlin d41d8cd98f00b204e9800998ecf8427e HEPL & KIPAC, Stanford University d41d8cd98f00b204e9800998ecf8427e Merida, Mexico

Uxmal + Tulum (Holiday Inn) 2007-07-07T12:41:00 2007-07-07T12:53:00 00:12 Recently, advances in VHE instrumentation have made the discovery of many new, predominantly Galactic, sources possible. Of these, a significant number can be identified as pulsar wind nebulae. It has long been known that pulsars can drive powerful winds of highly relativistic particles. These winds end in a termination shock from which high-energy particles with a wide spectrum of energies emerge. High-energy electrons and positrons among these particles give rise to two components of electromagnetic radiation: a low-energy component from synchrotron radiation and a high-energy component from inverse Compton upscattering of ambient photons. Details of the energy conversion mechanisms in the vicinity of pulsars are not well understood, nor is it known if all pulsars drive pulsar wind nebulae and emit high-energy radiation. Here we show that for a sample of pulsars in the central Milky Way, pulsars with large spin-down energy flux are with high probability associated with VHE gamma-ray sources. This implies that these pulsars emit on the order of 1% of their spin-down energy in tera electron volt gamma-ray energies. paper doc http://indico.nucleares.unam.mx/images/word.png word file ppt http://indico.nucleares.unam.mx/images/powerpoint.png powerpoint file pdf http://indico.nucleares.unam.mx/images/pdf_small.png pdf file odt http://indico.nucleares.unam.mx/images/writer.png writer file odp http://indico.nucleares.unam.mx/images/impress.png presentation file ods http://indico.nucleares.unam.mx/images/calc.png spreadsheet file other http://indico.nucleares.unam.mx/images/file_small.png unknown type file link http://indico.nucleares.unam.mx/images/link.png link 1 http://www.icrc2007.unam.mx/ link http://www.icrc2007.unam.mx/ doc http://indico.nucleares.unam.mx/images/word.png word file ppt http://indico.nucleares.unam.mx/images/powerpoint.png powerpoint file pdf http://indico.nucleares.unam.mx/images/pdf_small.png pdf file odt http://indico.nucleares.unam.mx/images/writer.png writer file odp http://indico.nucleares.unam.mx/images/impress.png presentation file ods http://indico.nucleares.unam.mx/images/calc.png spreadsheet file other http://indico.nucleares.unam.mx/images/file_small.png unknown type file link http://indico.nucleares.unam.mx/images/link.png link