On the absorption features in cosmic gamma-ray burst spectra recorded by the LILAS experiment

Details On the absorption features in cosmic gamma-ray burst spectra recorded by the LILAS experiment On the absorption features in cosmic gamma-ray burst spectra recorded by the LILAS experiment

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991p%26ss...39...67b&link_type=abstract

(Colloquium on Phobos-Mars Mission, Paris, France, Oct. 23-27, 1989, Proceedings. A91-29558 11-91) Planetary and Space Science (

Astronomy and Astrophysics

Astronomy

5

Energy Spectra, Gamma Ray Bursts, Spaceborne Astronomy, Spectral Emission, Astronomical Spectroscopy, Cyclotron Resonance, Line Spectra

Scientific paper

The Franco-Soviet LILAS experiment aboard the Phobos 2 probe was designed for investigation of cosmic gamma-ray bursts in the 3-1000 keV energy range. Two consecutive spectra, from the August 6, 1988 event, exhibit multiple absorption structures when the emission appears to soften progressively. The line energies at about 14 and 28 keV for the first spectrum, and at about 20, 40 and 60 keV for the second one, strongly support a cyclotron resonance mechanism in a greater than 10 to the 12th G magnetic field.

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