Metallicity dependence of HMXB populations

TL;DR

This study investigates how the number and brightness of high-mass X-ray binaries (HMXBs) depend on galaxy metallicity, finding they are significantly more numerous in low-metallicity galaxies, which impacts cosmic heating and ionization.

Contribution

It provides a quantitative analysis of the metallicity dependence of HMXB populations using Bayesian inference on compiled observational data, highlighting their increased prevalence in low-metallicity environments.

Findings

HMXBs are ten times more numerous per unit star formation in low-metallicity galaxies.

The luminosity of HMXBs shows minimal dependence on metallicity.

Results support the role of HMXBs in early universe heating and ionization.

Abstract

High-mass X-ray binaries (HMXBs) might have contributed a non-negligible fraction of the energy feedback to the interstellar and intergalactic media at high redshift, becoming important sources for the heating and ionization history of the Universe. However, the importance of this contribution depends on the hypothesized increase in the number of HMXBs formed in low-metallicity galaxies and in their luminosities. In this work we test the aforementioned hypothesis, and quantify the metallicity dependence of HMXB population properties. We compile from the literature a large set of data on the sizes and X-ray luminosities of HMXB populations in nearby galaxies with known metallicities and star formation rates. We use Bayesian inference to fit simple Monte Carlo models that describe the metallicity dependence of the size and luminosity of the HMXB populations. We find that HMXBs are typically ten times more numerous per unit star formation rate in low-metallicity galaxies (12 + log(O/H) < 8, namely < 20% solar) than in solar-metallicity galaxies. The metallicity dependence of the luminosity of HMXBs is small compared to that of the population size. Our results support the hypothesis that HMXBs are more numerous in low-metallicity galaxies, implying the need to investigate the feedback in the form of X-rays and energetic mass outflows of these high-energy sources during cosmic dawn.