Gamma rays from 'hidden' millisecond pulsars

Details Gamma rays from 'hidden' millisecond pulsars Gamma rays from 'hidden' millisecond pulsars

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...97..313t&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 97, no. 1, p. 313-316.

Astronomy and Astrophysics

Astronomy

3

Companion Stars, Emission Spectra, Gamma Rays, Light Emission, Pulsars, Radio Emission, Eclipsing Binary Stars, Evaporation, Gamma Ray Astronomy, Gamma Ray Observatory, Irradiation, Stellar Mass Accretion, Vaporizing

Scientific paper

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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