Astronomy and Astrophysics – Astrophysics
Scientific paper
May 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..dmp.g3005r&link_type=abstract
American Physical Society, 2002 Division of Atomic, Molecular and Optical , abstract #G3.005
Astronomy and Astrophysics
Astrophysics
Scientific paper
Theoretical models are constructed of the hard X-ray spectra resulting from electron capture by fully stripped Ne^10+ ions traversing the gases Ne, He, H_2, CO_2, and H_2O. The measured spectra are superpositions of individual lines of Ne^9+. An exact description of the radiative cascade is used. The initial excited populations that reproduce the measured spectra are derived and quantitative predictions of the energies and intensities of lines in the soft X-ray and extreme ultraviolet are made. These lines when observed will be powerful diagnostic probes of the capture mechanism and of the diverse range of laboratory and astrophysical plasmas in which it occurs.
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