A transient 77 keV emission feature from the Crab pulsar

Details A transient 77 keV emission feature from the Crab pulsar A transient 77 keV emission feature from the Crab pulsar

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982apj...253l..23s&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 253, Feb. 1, 1982, p. L23-L27. Navy-supported research.

Astronomy and Astrophysics

Astrophysics

26

Astronomical Spectroscopy, Emission Spectra, Pulsars, X Ray Sources, Crab Nebula, Line Spectra, Transient Response

Scientific paper

During a balloon-borne observation of the Crab pulsar, a transient
emission line at 77 keV, pulsed at the pulsar frequency, was detected
for the first 25 minutes of a 3 hour observation. This line then
disappeared, although the continuum remained unchanged. The implications
of a cyclotron origin of this feature are discussed.

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