An Updated Line List for Spectroscopic Investigation of G Stars- I: Redetermination of the Abundances in the Solar Photosphere

Yıl 2023, , 54 - 64, 21.12.2023

Timur Şahin , Mahmut Marışmak Nur Çınar , Selçuk Bilir

https://doi.org/10.26650/PAR.2023.00007

Öz

We propose a line list that may be useful for the abundance analysis of G-type stars in the wavelength range 4080 – 6780 Å. It is expected that the line list will be useful for surveys/libraries with overlapping spectral regions (e.g. ELODIE/SOPHIE libraries, UVES-580 setting of Gaia-ESO), and in particular for the analysis of F- and G-type stars in general. The atomic data are supplemented by detailed references to the sources. We estimated the Solar abundances using stellar lines and the high-resolution Kitt Peak National Observatory (KPNO) spectra of the Sun to determine the uncertainty in the log 𝑔 𝑓 values. By undertaking a systematic search that makes use of the lower excitation potential and 𝑔 𝑓 -values and using revised multiplet table as an initial guide, we identified 363 lines of 24 species that have accurate 𝑔 𝑓 -values and are free of blends in the spectra of the Sun and a Solar analogue star, HD 218209 (G6V), for which accurate and up-to-date abundances were obtained from both ELODIE and PolarBASE spectra of the star. For the common lines with the Gaia-ESO line list v.6 provided by the Gaia-ESO collaboration, we discovered significant inconsistencies in the 𝑔 𝑓 -values for certain lines of varying species.

Anahtar Kelimeler

Line, identification, Sun, abundances, fundamental parameters, Stars, individual (HD 218209)

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