Three-dimensional hydrodynamical simulations of surface convection in red giant 
stars: impact on spectral line formation and abundance analysis

Collet, R.; Asplund, M.; Trampedach, R.

doi:10.1051/0004-6361:20066321

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Three-dimensional hydrodynamical simulations of surface convection in red giant stars: impact on spectral line formation and abundance analysis

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Collet, R.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Collet, R., Asplund, M., & Trampedach, R. (2007). Three-dimensional hydrodynamical simulations of surface convection in red giant stars: impact on spectral line formation and abundance analysis. Astronomy & Astrophysics, 469(2), 687-706. doi:10.1051/0004-6361:20066321.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0011-AA4B-4

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