Table 1: Transitions and log  gf of Mult. 1: LW = Lambert & Warner (1968); Wiese = Wiese et al. (1969); BQZ = Biemont et al. (1993) and RL = Ryde & Lambert (2004).
  Transition $\lambda$ LW Wiese BQZ RL
    (nm)        
4s-4p $^5S^\circ$2-5P1 923.7538 -0.01 (*) 0.04 0.10 0.04
  $^5S^\circ$2-5P2 922.8093   0.23 0.26 0.32 0.25
  $^5S^\circ$2-5P3 921.2863   0.38 0.42 0.47 0.43
(*) This is the value given by Lambert & Warner (1968); Lambert & Luck (1978).
Nissen et al. (2004) use the value +0.01.

Source LaTeX | All tables | In the text

Article Contents
1 Introduction
2 Observational data
3 Atmospheric parameters
4 The S I spectrum
5 Analysis
6 Errors and sensitivity of abundances to stellar parameters
7 Sulphur abundances
8 Results
9 Discussion
10 Conclusions
References
Online Material
Appendix A: Remarks on individual stars
List of tables
List of figures