New Dimensions of Galactic Chemical Evolution

Abstract

Dramatic recent progress in understanding galactic chemical evolution (GCE) has been driven partly by direct observations of the distant past with HST and JWST of stellar abundances from giant high-resolution spectroscopic surveys (APOGEE, GALAH) and the complementary power of Gaia astrometry and photometry. Focusing on archaeology, I give a rapid-fire, and I hope synthesizing, review of work my collaborators and I have done on theoretical modeling and observational interpretation. I discuss (1) the interleaved but distinguishable roles of stellar scale astrophysics and galactic scale astrophysics in governing GCE, (2) the use of abundance ratio trends to empirically infer nucleosynthetic yields, (3) the uncertainty in the overall scale of yields and its degeneracy with the importance of galactic outflows, (4) the emergence of equilibrium in GCE, (5) the dimensionality of the stellar distribution in chemical abundance space, and (6) insights from chemical abundances on the early history of the Milky Way, including measurements of the intrinsic scatter of abundance ratios in metal-poor stars (-2 < [Fe/H] < -1), suggesting that a typical halo star at this metallicity is enriched by the products of $N\sim 50$ supernovae mixed over $\sim 10^5{M}_{\odot }$ of star-forming gas.

10 pp. running lightly over a lot of ground. Proceedings of IAU Symposium 377, Early Disk-Galaxy Formation: From JWST to the Milky Way, eds. F. Tabatabaei, B. Barbuy, and Y. Ting. Reactions welcome!

References in corpus (4)

• Birth of the Galactic Disk Revealed by the H3 Survey
• CNO dredge-up in a sample of APOGEE/Kepler red giants: Tests of stellar models and Galactic evolutionary trends of N/O and C/N
• The Iron Yield of Core-collapse Supernovae
• Strong Outflows and Inefficient Star Formation in the Reionization-era Ultra-faint Dwarf Galaxy Eridanus II

Cited by in corpus (1)

• Nuclear astrophysics