Is Geminga a very close neutron star binary?

Details Is Geminga a very close neutron star binary? Is Geminga a very close neutron star binary?

Nov 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.312...48n&link_type=abstract

Nature (ISSN 0028-0836), vol. 312, Nov. 1, 1984, p. 48-50.

Astronomy and Astrophysics

Astronomy

13

Binary Stars, Gamma Ray Astronomy, Neutron Stars, Stellar Rotation, X Ray Sources, Earth Magnetosphere, Pulsars, Stellar Evolution, Stellar Magnetic Fields, Stellar Models

Scientific paper

Geminga (2CG195+4) is one of the brightest sources in the sky at photon energies around 1 GeV. It has been tentatively identified with an unusual soft X-ray and optical object for which the γ-ray-to-X-ray-to-optical luminosity ratios are ≡106:103:1. This letter demonstrates that the observed properties of Geminga could be explained by a close binary model containing a neutron star if the system is located at a distance of 10 pc.

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