Published August 27, 2024 | Version v1
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Appendix D from "Gas-phase Fe/O and Fe/N Abundances in Star-Forming Regions. Relations Between Nucleosynthesis, Metallicity, and Dust"

Authors/Creators

  • 1. ROR icon Heidelberg University

Contributors

  • 1. Astronomisches Rechen-Institut
  • 2. ROR icon Instituto de Astrofísica de Canarias
  • 3. ROR icon Universidad Nacional Autónoma de México
  • 4. ROR icon Heidelberg University
  • 5. ROR icon University of Bologna
  • 6. ROR icon Max Planck Institute for Astrophysics
  • 7. ROR icon Ghent University
  • 8. Universidad de Granada

Description

Appendix D from 2024arXiv240806215M

Files

IRON_appendix_D-1.pdf

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Additional details

Identifiers

arXiv
arXiv:2408.06215

Related works

Is source of
Dataset: arXiv:2408.06215 (arXiv)

Dates

Accepted
2024-08-09
Accepted by Astronomy & Astrophysics

References

  • 2024arXiv240806215M