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

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DOI

    Maria Bergemann, Max Planck Inst Halbleiterlabor, Max Planck Society,
  • Remo Collet
  • Anish M. Amarsi, RSPAS, Australian National University, Mikhail Kovalev, Max Planck Inst Halbleiterlabor, Max Planck Society, Greg Ruchti, University Hospital, Lund University, Lund, Zazralt Magic, Nat 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