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Ultra-high-energy gamma-rays from Cygnus X-3Ultrahigh-energy gamma-ray emission with photon energies up to 20 PeV has been detected from the galactic X-ray source Cygnus X-3, implying acceleration of charged particles to even greater energies. A model for acceleration of particles to such energies in a binary containing an accreting neutron star with a magnetic field of about 100 MG is presented. The acceleration occurs in an accretion disk surrounding the neutron star, by an unipolar-inductor mechanism.
Document ID
19860062151
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Chanmugam, G.
(NASA Goddard Space Flight Center Greenbelt, MD; Louisiana State University, Baton Rouge, United States)
Brecher, K.
(NASA Goddard Space Flight Center Greenbelt, MD; Boston, University, MA, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Subject Category
Astrophysics
Accession Number
86A46889
Funding Number(s)
CONTRACT_GRANT: NSF AST-82-19598
Distribution Limits
Public
Copyright
Other

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