We present integral field spectroscopic observations of two local extremely metal-poor galaxies (XMPs), HSCJ1631+4426 and SDSSJ0811+4730, obtained with the Keck Cosmic Web Imager (KCWI) over 3545 − 5529 Ã at a spectral resolution of R ~ 3600, capturing bright nebular emission lines essential for determining gas-phase metallicity and chemical enrichment measurements. Using integrated spectra, we derive oxygen abundances of 12+log (O/H)=7.079± 0.010 and 6.926 ± 0.004, and elevated Fe/O ratios of log (Fe/O)=-1.57± 0.17 and −1.28 ± 0.07, for HSCJ1631+4426 and SDSSJ0811+4730 respectively. Each galaxy is fully contained within the 8.2” × 8.0” field of view, with 0.146” spaxels providing spatially resolved information. These measurements indicate unusually efficient iron enhancement at extremely low metallicity; Fe/O ratios approach or exceed solar despite oxygen abundances of only ~2% solar, inconsistent with enrichment from core-collapse supernovae alone or delayed Type Ia supernovae given the young ages of the systems. Comparison with chemical evolution models suggests rare, highly energetic explosions such as bright hypernovae and/or pair-instability supernovae are likely responsible. Our results reinforce the growing evidence that XMPs can reflect the nucleosynthetic processes of early energetic stellar explosions, serving as local laboratories for chemical enrichment pathways prevalent in the early Universe.
No takes yet. Share an insight, caveat, or question.
Myszka et al. (2026) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: