Table 1
Opacity tables available in Cesam2k20.
| Suffix | Solar abundances | High temperature | |||||||
|---|---|---|---|---|---|---|---|---|---|
| GN93 | GN93 (1) | OPAL | |||||||
| GS98_met | GS98 (2) | OPAL | |||||||
| GS98_phot | GS98 (2) | OPAL | |||||||
| AGS09_met | AGS09 (3,4) | OPAL | |||||||
| AGS09_phot | AGS09 (3) | OPAL | |||||||
| AGS09_met_OP_WICH | AGS09 (3,4) | OP | |||||||
| AGS09_phot_OP_WICH | AGS09 (3) | OP | |||||||
| AAG21_phot | AAG21 (5) | OPAL | |||||||
Notes. Opacity tables based on OPAL or OP tables, available in Cesam2k20. The name of each table is opa_yveline_ and a suffix. met stands for “meteoritic abundances” and phot for “photospheric abundances”. They are all matched linearly in the range log10 T = 4 ± 0.05 K, with Wichita opacity tables at low temperature. (1): Grevesse & Noels (1993); (2): Grevesse & Sauval (1998); (3): Asplund et al. (2009); (4): Serenelli et al. (2009) recommends taking photospheric abundances of Asplund et al. (2009) for valotile elements; (5): Asplund et al. (2021).
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