Identification lists of the far UV spectra of 7 solar chemical composition main sequence stars in the spectral range B2-B9.5

Details Identification lists of the far UV spectra of 7 solar chemical composition main sequence stars in the spectral range B2-B9.5 Identification lists of the far UV spectra of 7 solar chemical composition main sequence stars in the spectral range B2-B9.5

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...69....1r&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 69, no. 1, April 1987, p. 1-21. CNR-supported research.

Astronomy and Astrophysics

Astrophysics

4

Abundance, Early Stars, Main Sequence Stars, Stellar Spectra, Tables (Data), Ultraviolet Spectra, Far Ultraviolet Radiation, Line Spectra

Scientific paper

The authors present the identification lists for the far UV spectrum of 7 main-sequence stars with solar chemical composition, covering the spectral type range B2 - B9.5, to be used for comparison purposes in the analysis of UV spectra. The lists have been obtained by means of an automatic procedure developed by the authors consisting of the automatic recognition of the spectral features in the observed spectrum and of their identification via a list of theoretical lines whose central intensities have been computed starting from their atomic data and an appropriate model atmosphere. The procedure has been fine-tuned to select only the prominent features in the spectrum and to use only the strongest theoretical lines in the identification process; thus the identification lists do not contain those features to which no strong theoretical lines correspond.

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