Mon. Not. R. Astron. Soc., 488, 3492-3506 (2019/September-3)
Extremely metal-poor galaxies with HST/COS: laboratories for models of low-metallicity massive stars and high-redshift galaxies.
SENCHYNA P., STARK D.P., CHEVALLARD J., CHARLOT S., JONES T. and VIDAL-GARCIA A.
Abstract (from CDS):
Ultraviolet (UV) observations of local star-forming galaxies have begun to establish an empirical baseline for interpreting the rest-UV spectra of reionization-era galaxies. However, existing high-ionization emission line measurements at z > 6 ( W_C IV,0_ ≳20 Å) are uniformly stronger than observed locally ( W_C IV,0_ ≲2 Å), likely due to the relatively high metallicities (Z/Z☉ > 0.1) typically probed by UV surveys of nearby galaxies. We present new HST/COS spectra of six nearby (z < 0.01) extremely metal-poor galaxies (XMPs, Z/Z☉ <= 0.1) targeted to address this limitation and provide constraints on the highly uncertain ionizing spectra powered by low-metallicity massive stars. Our data reveal a range of spectral features, including one of the most prominent nebular C IV doublets yet observed in local star-forming systems and strong He II emission. Using all published UV observations of local XMPs to date, we find that nebular C IV emission is ubiquitous in very high specific star formation rate systems at low metallicity, but still find equivalent widths smaller than those measured in individual lensed systems at z > 6. Our moderate-resolution HST/COS data allow us to conduct an analysis of the stellar winds in a local nebular C IV emitter, which suggests that some of the tension with z > 6 data may be due to existing local samples not yet probing sufficiently high α/Fe abundance ratios. Our results indicate that C IV emission can play a crucial role in the JWST and ELT era by acting as an accessible signpost of very low metallicity (Z/Z☉ < 0.1) massive stars in assembling reionization-era systems.
© 2019 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society
stars: massive - galaxies: evolution - galaxies: stellar content - ultraviolet: galaxies
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