Phase distribution of the 0.44 MeV feature in the Crab pulsar spectrum

Details Phase distribution of the 0.44 MeV feature in the Crab pulsar spectrum Phase distribution of the 0.44 MeV feature in the Crab pulsar spectrum

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...97..321o&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 97, no. 1, p. 321-323.

Astronomy and Astrophysics

Astronomy

4

Gamma Ray Astronomy, Pulsars, Stellar Spectra, Balloon-Borne Instruments, Light Curve, Stellar Models

Scientific paper

On 1990 July 9, the balloon-borne experiment FIGARO II (0.15-4 MeV) observed the Crab region. The light-curve of PSR 0531 + 212 shows, in addition to the well-known two-peak structures, evidence for extra structures at absolute radio phases 0.1, 0.3, and 0.45 around the energy of 0.44 MeV. The phase-resolved spectroscopy confirms that an excess, compatible with a line-like feature, is present at these phase positions.

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