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NLTE line formation
Uppsala University, Disciplinary Domain of Science and Technology, Physics, Department of Physics and Astronomy, Theoretical Astrophysics.
2008 (English)In: Physica Scripta, ISSN 0031-8949, E-ISSN 1402-4896, Vol. T133, 014009- p.Article in journal (Refereed) Published
Abstract [en]

I review some of the present achievements and future challenges of non-local thermodynamicequilibrium (NLTE) line-formation calculations for solar-type stars. It is concluded that thefull potential of NLTE still remains to be tapped, in particular in view of the current transitionfrom one-dimensional (1D) hydrostatic to 3D hydrodynamic model atmospheres.

Place, publisher, year, edition, pages
Bristol: IOP , 2008. Vol. T133, 014009- p.
Keyword [en]
line formation, non-equilibrium, solar-type stars
National Category
Astronomy, Astrophysics and Cosmology
Research subject
Astronomy with specialization in Astrophysics
URN: urn:nbn:se:uu:diva-146237DOI: 10.1088/0031-8949/2008/T133/014009ISI: 000262583700011OAI: oai:DiVA.org:uu-146237DiVA: diva2:397775
23–27 June 2008, Uppsala, Sweden

Conference proceedings: A stellar journey. A symposium in celebration of Bengt Gustafsson's 65th birthday. 23–27 June 2008, Uppsala, Sweden. Eds. P.S. Barklem, A.J. Korn, B. Plez.

Available from: 2011-02-16 Created: 2011-02-15 Last updated: 2012-10-11Bibliographically approved

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Publisher's full texthttp://iopscience.iop.org/1402-4896/2008/T133

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