Search of a cyclotron line at 70 keV from Crab Nebula

Details Search of a cyclotron line at 70 keV from Crab Nebula Search of a cyclotron line at 70 keV from Crab Nebula

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980esasp.152..431u&link_type=abstract

In ESA European Rocket and Balloon Programs and Related Res. p 431-434 (SEE N81-10914 01-99)

Computer Science

Sound

Balloon Sounding, Crab Nebula, Cyclotron Radiation, X Ray Sources, Payloads, Proportional Counters, Pulsars, X Ray Astronomy, X Ray Telescopes

Scientific paper

An observation of the Crab Nebula was made during a transmediterranean balloon flight launched on August 26, 1979 from Milo Base (Sicily, Italy). The hard X-ray experiment (HXR 79) carried a payload consisting of two multiwire proportional counters having a geometric area of 900 sq cm each. A single transit scan of the source wa performed on the Crab Nebula region at a float altitude of 2.9 mbs. The preliminary results indicate the existence of an excess flux between 64 - 76 KeV above the expected value of l/e sq power law.

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