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Table 2

Stellar parameters and carbon abundances of our 3D CEMP model atmospheres.

Teff K log(g) dex [Fe/H] dex [C/Fe] dex A(C) dex Resolution Nx × Ny × Nz Size Mm
5750 4.5 −6 4 6.56 2402 × 120 5.2
5750 4.5 −5 3 6.56 2402 × 120 5.2
5750 4.5 −4 2 6.56 2402 × 120 5.1
5750 4.5 −3 1 6.56 2402 × 120 5.2
5750 4.5 −2 1 7.56 2402 × 120 5.4
5250 3.0 −6 4 6.56 2402 × 120 140
5250 3.0 −5 3 6.56 2402 × 120 140
5250 3.0 −4 2 6.56 2402 × 120 140
5250 3.0 −3 1 6.56 2402 × 120 150
5250 3.0 −2 1 7.56 2402 × 120 160

Notes. The level of C-enhancement varies from [C/Fe] = 1 (at [Fe/H] = −3) to [C/Fe] = 4(at [Fe/H] = −6). Here, Ni corresponds to the number of grid points in dimension i. In the last column, we provide the horizontal extend of the corresponding model atmosphere. Note that the vertical extend is half that number. For every CEMP model listed here, we generated a scaled-solar ([C/Fe] = 0) counterpart. For each model, convergence was achieved in less than 3500 CPU-h.

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