Accurate Spectroscopy of Intermediate and Late Spectral Types
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[1] J. Tomkin,et al. Light-element abundances in 20 F and G dwarfs. , 1985 .
[2] G. Stokes,et al. The pure rotation spectrum of OH and the solar oxygen abundance , 1984 .
[3] J. Hillman,et al. Thermal bifurcation in the upper photosphere inferred from heterodyne spectroscopy of OH rotational lines , 1984 .
[4] D. Murcray,et al. The pure rotation spectrum of the hydroxyl radical and the solar oxygen abundance , 1983 .
[5] J. Tomkin,et al. Evidence of non-LTE in photospheric lines of G and K giants , 1983 .
[6] Mitsuru Ebihara,et al. Solar-system abundances of the elements , 1982 .
[7] U. Becker,et al. Solar and meteoritic abundance of silicon , 1980 .
[8] H. Holweger,et al. The photospheric barium spectrum: Solar abundance and collision broadening of Baii lines by hydrogen , 1974 .
[9] Owen Gingerich,et al. The Harvard-Smithsonian reference atmosphere , 1971 .
[10] A. Goldman,et al. The 12C/13C and 16O/18O ratios in the solar photosphere , 1987 .
[11] W. Steenbock. Statistical Equilibrium of FE I/FE II in Cool Stars , 1985 .
[12] P. C. Keenan,et al. Cool stars with excesses of heavy elements , 1985 .
[13] E. Avrett,et al. Structure of the solar chromosphere. II - The underlying photosphere and temperature-minimum region , 1976 .
[14] B. Mason. Handbook of elemental abundances in meteorites , 1971 .