research

Cosmic Ray Accelerators in the Large Magellanic Cloud

Authors
Publication date
25 February 2010
Publisher
'IOP Publishing'
Doi
    View on arXiv

    Abstract

    I point out a correlation between gamma-ray emissivity and the historical star formation rate in the Large Magellanic Cloud ~12.5 Myr ago. This correlation bolsters the view that CRs in the LMC are accelerated by conglomerations of supernova remnants: i.e. superbubbles and supergiant shells.Comment: Research Not

      Similar works

      Full text

      thumbnail-image

      Available Versions

      Crossref

      redirect
      oaiinfo:doi/10.1088%2F0004-637x%2...
      Last time updated on 17/02/2019