Non-LTE line formation of Fe in late-type stars - III. 3D non-LTE analysis of metal-poor stars

Research output: Contribution to journal/Conference contribution in journal/Contribution to newspaperJournal articleResearchpeer-review

    A. M. Amarsi, Australian Natl Univ, Australian National University, Res Sch Astron & Astrophys, K. Lind, Max Planck Inst Astron, Max Planck Society, Uppsala Univ, Uppsala University, Dept Phys & Astron, Theoret Astrophys, M. Asplund, Australian Natl Univ, Australian National University, Res Sch Astron & Astrophys, P. S. Barklem, Uppsala Univ, Uppsala University, Dept Phys & Astron, Theoret Astrophys,
  • R. Collet
Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume463
Issue number2
Pages (from-to)1518-1533
Number of pages16
ISSN0035-8711
DOIs
StatePublished - 1 Dec 2016

    Research areas

  • line: formation, radiative transfer, methods: numerical, stars: abundances, stars: atmospheres, RELATIVE OSCILLATOR-STRENGTHS, GALACTIC CHEMICAL EVOLUTION, NEUTRAL HYDROGEN COLLISIONS, RADIATIVE-TRANSFER CODE, ATOM-ATOM COLLISIONS, COOL DWARF STARS, R-MATRIX METHOD, STELLAR ATMOSPHERES, MODEL ATMOSPHERES, CROSS-SECTIONS

See relations at Aarhus University Citationformats

ID: 107707260