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Pulsar counterparts of gamma-ray sources

Name: Pulsar counterparts of gamma-ray sources
Keywords: Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jan 1997Embargo end date: 01 Jan 1997Publisher:AIPJournal:AIP Conference Proceedings

Authors: Giovanni F. Bignami; P. A. Caraveo;

doi: 10.1063/1.54036 , 10.48550/arxiv.astro-ph/9711070

arXiv: http://arxiv.org/abs/astro-ph/9711070

Pulsar counterparts of gamma-ray sources

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Abstract

The EGRET catalogue of unidentified X-ray sources has more objects along the galactic disk than at high galactic latitude, where identifications are comparatively easier. On the other hand, the Egret/GRO mission has already identified several known radio pulsars as gamma-ray sources as well as discovering Geminga's nature as a pulsar. If Geminga is not a unique case, as it is very likely not to be, than other galactic sources could, in fact, be radio quiet isolated neutron stars. For these, the identification work is extremely difficult and should anyway start from high resolution X-ray/optical data.

6 pages, LaTeX, macro aipproc.sty

Related Organizations

Agenzia Spaziale Italiana
Italy

Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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Related to Research communities

NEANIAS Space Research Community