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

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons20167

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons26319

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons16270

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

http://pubman.mpdl.mpg.de/cone/persons/resource/persons20203

Magic,  Z.
Stellar Astrophysics, MPI for Astrophysics, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons16172

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

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Citation

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