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Gamma rays from hidden millisecond pulsarsThe properties were studied of a new class of gamma ray sources consisting of millisecond pulsars totally or partially surrounded by evaporating material from irradiated companion stars. Hidden millisecond pulsars offer a unique possibility to study gamma ray, optical and radio emission from vaporizing binaries. The relevance of this class of binaries for GRO observations and interpretation of COS-B data is emphasized.
Document ID
19920012660
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Tavani, Marco (Lawrence Livermore National Lab. Livermore, CA, United States)
Date Acquired
September 6, 2013
Publication Date
February 1, 1992
Publication Information
Publication: NASA. Goddard Space Flight Center, The Compton Observatory Science Workshop
Subject Category
Space Radiation
Accession Number
92N21903
Funding Number(s)
CONTRACT_GRANT: GRO-90-29
CONTRACT_GRANT: GRO-PFP-91-23
CONTRACT_GRANT: W-7405-ENG-48
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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