Three-dimensional hydrodynamical simulations of red giant stars: semi-global 
models for interpreting interferometric observations

Chiavassa, A.; Collet, R.; Casagrande, L.; Asplund, M.

doi:10.1051/0004-6361/201015507

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Three-dimensional hydrodynamical simulations of red giant stars: semi-global models for interpreting interferometric observations

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Chiavassa, A.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons16270

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

/persons/resource/persons16258

Casagrande, L.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons16172

Asplund, M.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

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Chiavassa, A., Collet, R., Casagrande, L., & Asplund, M. (2010). Three-dimensional hydrodynamical simulations of red giant stars: semi-global models for interpreting interferometric observations. Astronomy & Astrophysics, 524:, pp. 1-13. doi:10.1051/0004-6361/201015507.

引用: https://hdl.handle.net/11858/00-001M-0000-0010-9123-3

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