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Cyclotron scattering lines in gamma-ray burst spectraIf cyclotron scattering, rather than absorption, is responsible for the line features observed recently in two gamma-ray burst spectra (Murakami et al., 1988), then the second and higher harmonics are due to resonant scattering events that excite the electron to Landau levels above the ground state. Here, relativistic Compton scattering cross sections are used to estimate the expected ratio of third to second harmonics in the presence of Doppler broadening. At the field strength (1.7 TG) required to give first and second harmonics at 19 keV and 38 keV, there should be no detectable third harmonic in the spectrum.
Document ID
19890039679
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Harding, Alice K.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Preece, Robert D.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
March 1, 1989
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters
Volume: 338
ISSN: 0004-637X
Subject Category
Space Radiation
Accession Number
89A27050
Distribution Limits
Public
Copyright
Other

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