Non-local Thermodynamic Equilibrium Stellar Spectroscopy with 1D and <3D > Models. I. Methods and Application to Magnesium Abundances in Standard Stars

Research output: Research - peer-reviewJournal article

DOI

  • Maria Bergemann
    Maria BergemannMax Planck Inst Halbleiterlabor, Max Planck Society
  • Remo Collet
  • Anish M. Amarsi
    Anish M. AmarsiRSPAS, Australian National University
  • Mikhail Kovalev
    Mikhail KovalevMax Planck Inst Halbleiterlabor, Max Planck Society
  • Greg Ruchti
    Greg RuchtiUniversity Hospital, Lund University, Lund
  • Zazralt Magic
    Zazralt MagicNat Hist Museum Denmark, Ctr Excellence GeoGenet
Original languageEnglish
Article number15
JournalAstrophysical Journal
Volume847
Issue number1
Number of pages19
ISSN0004-637X
DOIs
StatePublished - 20 Sep 2017

    Research areas

  • galaxies: abundances, line: formation, radiative transfer, stars: abundances, stars: late-type, METAL-POOR STARS, LTE LINE FORMATION, NEUTRAL HYDROGEN-ATOMS, MG-I, TRANSITION-PROBABILITIES, OSCILLATOR-STRENGTHS, RADIATIVE LIFETIMES, SOLAR GRANULATION, SPECTRAL-LINES, MAFAGS-OS

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ID: 117945983