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Monthly notices of the Royal Astronomical Society, ISSN 0035-8711, 09/2016, Volume 461, Issue 3, pp. 3274 - 3295
We present a model of the early chemical composition and elemental abundances of planetary atmospheres based on the cumulative gaseous chemical species that are accreted on to planets forming by core... 
Planets and satellites: atmospheres | Protoplanetary discs | Planets and satellites: formation | Planets and satellites: composition | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Extrasolar planets | Accretion disks | Star & galaxy formation | Astronomy | Planetary atmospheres | Accretion | Mixing ratios | Planet formation | Planetary evolution | Gas giant planets | Physics - Earth and Planetary Astrophysics
Journal Article
Astronomy and astrophysics (Berlin), ISSN 0004-6361, 02/2017, Volume 598, p. L10
.... Model atmospheres were computed in 3D for three distinct CNO chemical compositions using the (COBOLD... 
Line: formation | Hydrodynamics | Radiative transfer | Molecular processes | Stars: chemically peculiar | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Physics - Solar and Stellar Astrophysics
Journal Article
Monthly notices of the Royal Astronomical Society, ISSN 1365-2966, 11/2012, Volume 427, Issue 1, pp. 27 - 49
...) line formation calculations for Fe were performed using 1D hydrostatic marcs and mafags-os model atmospheres, as well as the spatial and temporal average stratifications from full 3D hydrodynamical... 
line: formation | line: profiles – radiative transfer | atomic data | stars: abundances | Line: formation | Stars: abundances | Atomic data | Line: profiles - radiative transfer | Physical Sciences | Astronomy & Astrophysics | Science & Technology | Models | Star & galaxy formation | Stars & galaxies | Atmosphere
Journal Article