Non-LTE line formation of Fe in late-type stars – I. Standard stars with 1D and 
〈3D〉 model atmospheres

Bergemann, Maria; Lind, K.; Collet, R.; Magic, Z.; Asplund, M.

doi:10.1111/j.1365-2966.2012.21687.x

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Non-LTE line formation of Fe in late-type stars – I. Standard stars with 1D and 〈3D〉 model atmospheres

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Bergemann, Maria
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons26319

Lind, K.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

/persons/resource/persons16270

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

/persons/resource/persons20203

Magic, Z.
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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Bergemann, M., Lind, K., Collet, R., Magic, Z., & Asplund, M. (2012). Non-LTE line formation of Fe in late-type stars – I. Standard stars with 1D and 〈3D〉 model atmospheres. Monthly Notices of the Royal Astronomical Society, 427(1), 27-49. doi:10.1111/j.1365-2966.2012.21687.x.

Cite as: https://hdl.handle.net/11858/00-001M-0000-000E-7859-1

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