X-ray line emission from Capella

Details X-ray line emission from Capella X-ray line emission from Capella

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stin...7929124h&link_type=abstract

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Emission Spectra, Line Spectra, Stars, X Ray Fluorescence, Coronas, Iron, Magnesium, Silicon, Sulfur, X Ray Spectra

Scientific paper

X-ray emission line components from Mg, Si, S and Fe were unambiguously detected from Capella with the Solid-State Spectrometer onboard the Einstein Observatory. The X-ray spectrum is inconsistent with an isothermal corona, and requires components between 6,000,000 K and at least 24,000,000 K for an adequate fit. An inhomogeneous corona in which the X-ray emitting plasma is confined to magnetically-contained loops appears to be reconcilable with all of the experimental evidence.

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