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astro-ph2001★ 4 cited

An astrophysical oscillator strength for the SII 94.7 nm resonance line and S abundances in DLAs

P. Bonifacio, E. Caffau, M. Centurion +2

By using UV spectra for the O star HD 93521 taken with the ORFEUS II echelle spectrograph, we determine an ``astrophysical'' f value for the SII 94.7 nm line: f = 0.00498 (+0.00172…