Log(gf) for singly-ionized elements of the iron group. II

Details Log(gf) for singly-ionized elements of the iron group. II Log(gf) for singly-ionized elements of the iron group. II

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.115...61m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 115, no. 1, Oct. 1985, p. 61-70. Research supported by SECYT.

Astronomy and Astrophysics

Astrophysics

3

Metal Ions, Metallicity, Stellar Composition, Stellar Spectra, Transition Metals, Transition Probabilities, Accuracy, Correction, Oscillator Strengths, Photosphere, Solar Atmosphere

Scientific paper

An attempt is made to extend existing lists of log(gf) values for singly ionized elements of the iron group, introducing systematic corrections to Warner's determinations (Warner, 1967). The suggested corrections shift Warner's log(gf) system in Kurucz-Peytremann's system. Warner's corrected log(gf) are compared with other modern values, and results are found to be quite satisfactory for iron although not as good for titanium. Abundances consistent with those currently accepted are obtained for the iron group in the solar photosphere if the proposed corrected log(gf) values are used.

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