Journal article Open Access

Evidence for Muon Production by Particles from Cygnus X-3

Marshak, M. L.; Bartelt, J.; Courant, H.; Heller, K.; Joyce, T.; Peterson, E. A.; Ruddick, K.; Shupe, M.; Ayres, D. S.; Dawson, J.; Fields, T.; May, E. N.; Price, L. E.; Sivaprasad, K.


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  <titles>
    <title>Evidence for Muon Production by Particles from Cygnus X-3</title>
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  <publisher>Zenodo</publisher>
  <publicationYear>1985</publicationYear>
  <dates>
    <date dateType="Issued">1985-05-13</date>
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  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/1233841</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1103/physrevlett.54.2079</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="http://creativecommons.org/publicdomain/zero/1.0/legalcode">Creative Commons Zero v1.0 Universal</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">We have observed underground cosmic-ray muons, corresponding to a secondary flux of ∼7×10−11 cm−2 s−1, at a depth of 1800 m water equivalent, which appear to be initiated by Cygnus X-3. This identification is based on both direction and phase coherence. The existence of such secondary muons conflicts with the current understanding of photon cascades and/or the nature and location of Cygnus X-3.</description>
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