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2005ApJ...625.1045L - Astrophys. J., 625, 1045-1061 (2005/June-1)

Emission-line spectra of S VII-S XIV in the 20-75 Å wavelength region.

LEPSON J.K., BEIERSDORFER P., BEHAR E. and KAHN S.M.

Abstract (from CDS):

As part of a larger project to complete a comprehensive catalog of astrophysically relevant emission lines in support of new-generation X-ray observatories using the Lawrence Livermore electron beam ion traps EBIT-I and EBIT-II, we present observations of sulfur lines in the soft X-ray and extreme-ultraviolet regions. Our database includes wavelength measurements with standard errors, relative intensities, and line assignments for 127 transitions of S VII through S XIV between 20 and 75 Å. The experimental data are complemented with a full set of calculations using the Hebrew University Lawrence Livermore Atomic Code (HULLAC). A comparison of the laboratory data with Chandra measurements of Procyon allows us to identify S VII-S XI lines.

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Journal keyword(s): Line: Identification - Methods: Analytical - Methods: Laboratory - Stars: Coronae - Stars: Individual: Name: Procyon

Simbad objects: 1

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