Feature in the Crab Pulsar gamma-ray spectrum

Details Feature in the Crab Pulsar gamma-ray spectrum Feature in the Crab Pulsar gamma-ray spectrum

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991aipc..232..335p&link_type=abstract

IN: Gamma-ray line astrophysics; Proceedings of the International Symposium, Paris, France, Dec. 10-13, 1990 (A92-43619 18-90).

Astronomy and Astrophysics

Astrophysics

2

Crab Nebula, Gamma Ray Spectra, Light Curve, Pulsars, Balloon-Borne Instruments, Emission Spectra, Gamma Ray Observatory

Scientific paper

A complete analysis has been undertaken of the pulsar light curve obtained during the third flight of the French-Italian Gamma-Ray Observatory II (FIGARO II) experiment for the Crab Pulsar, in order to expand on the earlier, but still ambiguous, discovery of a line in the vicinity of 450 keV. FIGARO II is a balloon-borne, large-area noncollimated photon detector designed for observation of sources with well-defined time signatures.

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