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Koch-Miramond, L.; Rocchia, R.; Becker, R.H.
CEA Centre d'Etudes Nucleaires de Saclay, 91 - Gif-sur-Yvette (France). Inst. de Recherche Fondamentale (IRF)1985
CEA Centre d'Etudes Nucleaires de Saclay, 91 - Gif-sur-Yvette (France). Inst. de Recherche Fondamentale (IRF)1985
AbstractAbstract
[en] The remnant G 29.7 - 0.3 has been studied intensively. The present paper shows Exosat results obtained with the imaging instrument and the medium energy proportional counters. Assuming that the featureless power-law spectrum obtained in the 2 to 10 keV range is synchrotron radiation from relativistic electrons, one derives constraints on magnetic field strength and age of the nebula. The energy spectra of the electrons responsible for the emission in the radio and X-ray range are discussed
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Aug 1985; 4 p; 19. International cosmic ray conference; La Jolla, CA (USA); 11-23 Aug 1985
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Report
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Conference
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