Measuring the proper motion of the Geminga pulsar using γ-ray data.

Details Measuring the proper motion of the Geminga pulsar using γ-ray data. Measuring the proper motion of the Geminga pulsar using γ-ray data.

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995acaps..15..289c&link_type=abstract

Acta Astrophys. Sin., Vol. 15, No. 3, p. 289 - 291

Astronomy and Astrophysics

Astrophysics

Pulsars: Proper Motions, Gamma-Ray Pulsars: Optical Counterparts, Gamma-Ray Pulsars: Positions

Scientific paper

The authors have measured the right ascension of Geminga at different epochs by comparing the absolute phases between the different γ-ray observations. These values show that the right-ascension component of the proper motion of Geminga is 0.226±0.03 arcsec per year, which is consisten with that of G″ the most probable optical counterpart, thus independently confirming the correspondence between G″and Geminga.

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