Spectral Signatures of Population III and Envelope-stripped Stars in Galaxies at the Epoch of Reionization

2021/02/16 by Elizabeth Berzin, Amy Secunda, Renyue Cen +5
Physics and Astronomy · #Astronomy #Astronomy and Astrophysical Research #Astrophysics #Astrophysics and Star Formation Studies #Galaxies: Formation, Evolution, Phenomena #Galaxy #Luminosity #Luminosity function #Metallicity #Physics #Population #Redshift #Reionization #Star formation #Stars #Stellar, planetary, and galactic studies #astro-ph.GA

paper · pdf · doi:10.3847/1538-4357/ac0af6

16 pages, 9 figures. Accepted to ApJ

openalex publication_date 2021/02/16 · arxiv created 2021/08/10 · arxiv updated 2021/09/08 · openalex created_date 2021/09/13 · openalex updated_date 2026/08/05

Abstract

While most simulations of the epoch of reionization have focused on single-stellar populations in star-forming dwarf galaxies, products of binary evolution are expected to significantly contribute to emissions of hydrogen-ionizing photons. Among these products are stripped stars (or helium stars), which have their envelopes stripped from interactions with binary companions, leaving an exposed helium core. Previous work has suggested these stripped stars can dominate the LyC photon output of high-redshift low luminosity galaxies. Other sources of hard radiation in the early universe include zero-metallicity Population III stars, which may have similar SED properties to galaxies with radiation dominated by stripped star emissions. Here, we use two metrics (the power-law exponent over wavelength intervals 240-500 \rA, 600-900 \rA, and 1200-2000 \rA, and the ratio of total luminosity in FUV wavelengths to LyC wavelengths) to compare the SEDs of simulated galaxies with only single-stellar evolution, galaxies containing stripped stars, and galaxies containing Population III stars, with four different IMFs. We find that stripped stars significantly alter the SEDs in the LyC range of galaxies at the epoch of reionization. SEDs in galaxies with stripped stars present have lower power-law indices in the LyC range and lower FUV to LyC luminosity ratios. These differences in SEDs are present at all considered luminosities (M_UV > -15, AB system), and are most pronounced for lower luminosity galaxies. We also find that SEDs of galaxies with stripped stars and Pop III stars are distinct from each other for all tested IMFs.

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