The evolution of accretor stars in binary systems due to accretion of increasingly helium-rich material

TL;DR

This paper models how accreting helium-rich material in binary systems alters stellar structure and evolution, revealing commonality and implications for astrophysical phenomena.

Contribution

It demonstrates the impact of helium-rich accretion on star properties and evolution, using detailed models and population estimates.

Findings

Helium-rich accretion makes stars hotter and more luminous.

Approximately 23% of massive binaries experience helium-rich mass transfer.

Implications for mass discrepancy, ionizing photon production, and galaxy modeling.

Abstract

The recent discovery of examples of intermediate-mass helium stars have offered new insights into interacting binaries. These observations will allow significant improvements in our understanding of helium stars. However, in the creation of these stars their companions may accrete a significant amount of helium-rich stellar material. These creates stars with unusual composition profiles -- stars with helium-rich cores, hydrogen-rich lower envelopes and a helium-rich outer envelope. Thus the mean molecular weight reaches a minimum in the the middle of the star rather than continuously decreasing outwards in mass. To demonstrate this structure we present Cambridge STARS model calculations of an example interacting binary systems where the helium-rich material is transferred, and compare it to one where the composition of the accreted mass is fixed to the companion's surface composition. We show that the helium-rich material leads to the accretor being 0.2 dex hotter and 0.15 dex more luminous than models where the composition is not helium rich. We use a simple BPASS v2.2 population model to estimate that helium-rich mass transfer occurs in 23 per cent of massive binaries that undergo mass transfer. This suggests this is a common process. This binary process has implications for the discrepancy between spectroscopic and gravitational masses of stars, the production of ionizing photons and possibly the modelling of high redshift galaxies.