The Astrophysical Journal (Jan 2024)

CLASSY. IX. The Chemical Evolution of the Ne, S, Cl, and Ar Elements

  • Karla Z. Arellano-Córdova,
  • Danielle A. Berg,
  • Matilde Mingozzi,
  • Bethan L. James,
  • Noah S. J. Rogers,
  • Evan D. Skillman,
  • Fergus Cullen,
  • Ryan K. Alexander,
  • Ricardo O. Amorín,
  • John Chisholm,
  • Matthew Hayes,
  • Timothy Heckman,
  • Svea Hernandez,
  • Nimisha Kumari,
  • Claus Leitherer,
  • Crystal L. Martin,
  • Michael Maseda,
  • Themiya Nanayakkara,
  • Kaelee Parker,
  • Swara Ravindranath,
  • Allison L. Strom,
  • Fiorenzo Vincenzo,
  • Aida Wofford

DOI
https://doi.org/10.3847/1538-4357/ad34cf
Journal volume & issue
Vol. 968, no. 2
p. 98

Abstract

Read online

To study the chemical evolution across cosmic epochs, we investigate Ne, S, Cl, and Ar abundance patterns in the Cosmic Origins Spectrograph Legacy Archive Spectroscopic SurveY (CLASSY). CLASSY comprises local star-forming galaxies (SFGs; 0.02 8.5, likely due to ICFs. Thus, the applicability of the ICFs to integrated spectra of galaxies could bias results, underestimating true abundance ratios. Using CLASSY as a local reference, we assess the evolution of Ne/O, S/O, and Ar/O in galaxies at z > 3, finding no cosmic evolution of Ne/O, while the lack of direct abundance determinations for S/O and Ar/O can bias the interpretation of the evolution of these elements. We determine the fundamental metallicity relationship (FMR) for CLASSY and compare to the high-redshift FMR, finding no evolution. Finally, we perform the first mass–neon relationship analysis across cosmic epochs, finding a slight evolution to high Ne at later epochs. The robust abundance patterns of CLASSY galaxies and their broad range of physical properties provide essential benchmarks for interpreting the chemical enrichment of the early galaxies observed with the JWST.

Keywords