Geminga gamma pulsar light curve at energies of 400-4000 MeV on the basis of data of the Gamma-1 telescope

Details Geminga gamma pulsar light curve at energies of 400-4000 MeV on the basis of data of the Gamma-1 telescope Geminga gamma pulsar light curve at energies of 400-4000 MeV on the basis of data of the Gamma-1 telescope

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993astl...19..229a&link_type=abstract

Astronomy Letters, Vol. 19, p. 229-230; Pis'ma v Astronomicheskij Zhurnal (ISSN 0320-0108), vol. 19, no. 7, p. 579-582. In Russ

Astronomy and Astrophysics

Astronomy

4

Energy Spectra, Gamma Ray Telescopes, Light Curve, Pulsars, Power Series, Pulsed Radiation

Scientific paper

Data of the Gamma-1 telescope are used to obtain the Geminga light curve, with two peaks separated by 0.5 +/- 0.3 of the period. The light curve is pronounced for gamma quanta with energies higher than 400 MeV. The upper limit for the pulsed flux at energies of 50-300 MeV is 6 x 10 exp 7/sq cm s. At energies higher than 300 MeV, the pulsed component power law spectrum has a spectral slope of 1.1 + 1.1/-0.3 and an integral flux of (1.1 +/- 0.3) x 10 exp -6/sq cm/s.

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