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20042026
most citedGaia Data Release 2. Summary of the contents and survey properties

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astro-ph2004★ 268 cited

Line formation in solar granulation VI. [C I], C I, CH and C2 lines and the photospheric C abundance

M. Asplund, N. Grevesse, A. J. Sauval +2

The solar photospheric carbon abundance has been determined from [C I], C I, CH vibration-rotation, CH A-X electronic and C2 Swan electronic lines by means of a time-dependent, 3D,…