EXOSAT observation of the candidate X-ray counterpart of Geminga

Details EXOSAT observation of the candidate X-ray counterpart of Geminga EXOSAT observation of the candidate X-ray counterpart of Geminga

Aug 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.310..481c&link_type=abstract

Nature (ISSN 0028-0836), vol. 310, Aug. 9, 1984, p. 481-483.

Astronomy and Astrophysics

Astronomy

12

Exosat Satellite, Gamma Ray Astronomy, X Ray Sources, Channel Multipliers, Time Measurement, Variable Stars

Scientific paper

During a search for X-ray counterparts of the COS B ≥100 MeV γ-ray sources, observations using the Einstein Observatory revealed a new X-ray source, 1E0630+178, inside the ≡1/2 square degree error box of the γ-ray source 2CG195+4, 'Geminga'. This source has been proposed as the X-ray counterpart of Geminga. The region of Geminga was observed with the ESA Exosat satellite on 9 - 10 September 1983. This letter presents time profiles of the X-ray emission observed with the Channel Multiplier Arrays.

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