Supernova remnants in molecular clouds: on cosmic ray electron spectra

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dc.creatorOstrowski, M.
dc.date1998-12-23
dc.date.accessioned2026-07-07T02:29:48Z
dc.date.available2026-07-07T02:29:48Z
dc.descriptionThe particle acceleration process at a shock wave, in the presence of the second-order Fermi acceleration in the turbulent medium near the shock, is discussed as an alternative explanation for the observed flat synchrotron spectra of supernova remnants (SNRs) in molecular clouds. We argue that medium Alfvén Mach number shocks considered by Chevalier (1999, ApJ, in press) for such SNRs can naturally lead to the observed spectral indices.
dc.descriptionLaTeX (4 pages, 2 postscript figures); A&A, accepted
dc.identifierhttps://arxiv.org/abs/astro-ph/9812433
dc.identifierhttp://arxiv.org/abs/astro-ph/9812433
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13616
dc.subjectAstrophysics
dc.titleSupernova remnants in molecular clouds: on cosmic ray electron spectra
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