Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995a%26a...296..233h&link_type=abstract
Astronomy and Astrophysics, v.296, p.233
Astronomy and Astrophysics
Astrophysics
84
Sun: Abundances, Atomic Data
Scientific paper
We examine the critical remarks by Blackwell, Lynas-Gray & Smith (1995; A&A, this issue). Points discussed in detail include equivalent widths, oscillator strengths, microturbulence, damping, and models of the solar photosphere. In addition, we present new results based on the Fe i oscillator strengths of Bard & Kock (1994). The sample of weak solar lines, which are the most reliable abundance indicators, is greatly increased. The result is fully consistent with our earlier determinations based on lines of Fe i and Fe ii.
Bard A.
Holweger Hartmut
Kock Manfred
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