Line feature around 73 keV from the Crab Nebula

Details Line feature around 73 keV from the Crab Nebula Line feature around 73 keV from the Crab Nebula

Jan 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...252..172m&link_type=abstract

Astrophysical Journal, Part 1, vol. 252, Jan. 1, 1982, p. 172-178.

Astronomy and Astrophysics

Astronomy

23

Astronomical Spectroscopy, Balloon-Borne Instruments, Crab Nebula, Cyclotron Radiation, Gamma Ray Astronomy, X Ray Sources, Data Reduction, Line Spectra, Proportional Counters, Pulsars, Spectrum Analysis, X Ray Spectra

Scientific paper

Observational data for the Crab Nebula obtained with a balloon-borne, multiwire high-pressure xenon proportional counter indicate an X-ray spectrum line feature at approximately 73 keV. Source continuous emission fits a power law of 16.5E to the -2.3, and a line intensity of 0.005 + or - 0.0015 photons/sq cm per sec is arrived at, for an equivalent width of 3 keV. These results are discussed in light of the possibility of a cyclotron emission process serving as the mechanism for the observed line.

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