Issue |
A&A
Volume 687, July 2024
|
|
---|---|---|
Article Number | A294 | |
Number of page(s) | 7 | |
Section | Stellar structure and evolution | |
DOI | https://doi.org/10.1051/0004-6361/202450341 | |
Published online | 23 July 2024 |
Constraining the helium-to-metal enrichment ratio ΔY/ΔZ from main-sequence binary stars
Theoretical analysis of the accuracy and precision of the age and helium abundance estimates
1
Dipartimento di Fisica “Enrico Fermi”, Università di Pisa, Largo Pontecorvo 3, 56127 Pisa, Italy
e-mail: valle@df.unipi.it
2
INFN, Sezione di Pisa, Largo Pontecorvo 3, 56127 Pisa, Italy
Received:
12
April
2024
Accepted:
13
May
2024
Aims. We aim to investigate the theoretical possibility of accurately determining the helium-to-metal enrichment ratio ΔY/ΔZ from precise observations of double-lined eclipsing binary systems.
Methods. Using Monte Carlo simulations, we drew synthetic binary systems with masses between 0.85 and 1.00 M⊙ from a grid of stellar models. Both stars were sampled from a grid with ΔY/ΔZ = 2.0, with a primary star at 80% of its main-sequence evolution. Subsequently, a broader grid with ΔY/ΔZ from 1.0 to 3.0 was used in the fitting process. To account for observational uncertainties, two scenarios were explored: S1, with realistic uncertainties of 100 K in temperature and 0.1 dex in [Fe/H]; and S2, with halved uncertainties. We repeated the simulation at two baseline metallicities: [Fe/H] = 0.0 and −0.3.
Results. The posterior distributions of ΔY/ΔZ revealed significant biases. The distributions were severely biased towards the edge of the allowable range in the S1 error scenario. The situation only marginally improved when considering the S2 scenario. The effect is due to the impact of changing ΔY/ΔZ in the stellar effective temperature and its interplay with [Fe/H] observational error, and it is therefore not restricted to the specific fitting method. Despite the presence of these systematic discrepancies, the age of the systems were recovered unbiased with 10% precision.
Conclusions. Our findings indicate that the observational uncertainty in effective temperature and metallicity significantly hinders the accurate determination of the ΔY/ΔZ parameter from main-sequence binary systems.
Key words: methods: statistical / binaries: eclipsing / stars: evolution / stars: fundamental parameters / stars: interiors
© The Authors 2024
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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