NASA NTRS ยท 19920012660
Gamma rays from hidden millisecond pulsars
Abstract
The 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.
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Tavani, Marco. 1992-02-01. Gamma rays from hidden millisecond pulsars. https://ntrs.nasa.gov/citations/19920012660
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