BBXRT Observations of Fe Lines in CAS A

Details BBXRT Observations of Fe Lines in CAS A BBXRT Observations of Fe Lines in CAS A

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aas...182.1907s&link_type=abstract

American Astronomical Society, 182nd AAS Meeting, #19.07; Bulletin of the American Astronomical Society, Vol. 25, p.820

Astronomy and Astrophysics

Astronomy

Scientific paper

The Broad Band X-Ray Telescope (BBXRT) observations of the supernova remnant(SNR) Cas A provided the first examination of the region of the x-ray spectrum around 6 keV with a spectrometer with sufficient resolution (FWHM circa 180 eV) to partially resolve the Fe lines. The observed line complex is inconsistent with a single narrow line. Additionally, we have not been able to obtain a good fit with models of the X-ray emission from a Sedov-type SNR. We will discuss what types of combinations of emissions could be consistent with the data

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