Search for Gamma Ray Line Emission from SS433 in the SMM GRS Data Base

Details Search for Gamma Ray Line Emission from SS433 in the SMM GRS Data Base Search for Gamma Ray Line Emission from SS433 in the SMM GRS Data Base

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...180.0402g&link_type=abstract

American Astronomical Society, 180th AAS Meeting, #04.02; Bulletin of the American Astronomical Society, Vol. 24, p.732

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Gamma ray spectra of SS433 obtained by the Gamma Ray Spectrometer aboard the Solar Maximum Mission satellite during 1980-1989 were examined for evidence of Doppler shifted line emission. The main emphasis, using both 3-day and 9-day integrations, was on the 1.368 MeV magnesium-24 line suggested by Lamb et al. (1983, Nature, 305,37). This work completes the examination of the SMM data base on SS433, augmenting and extending the study of Geldzahler et al. (1989, Ap.J., 342, 1123). The results are examined in the context of the models of gamma ray emission from SS433 published by Ramaty et al. (1984, Ap.J., 283, L13) and Boyd et al. (1984, Ap.J.,276, L9). This work was supported by NASA grant NAS 5-26954 at the Institute for Computational Sciences and Informatics, George Mason University.

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