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- W4311454664 abstract "Context. SMSS J160540.18−144323.1 is the carbon-enhanced metal-poor (CEMP) star with the lowest iron abundance ever measured, [Fe/H] = −6.2, which was first reported with the SkyMapper telescope. The carbon abundance is A (C)≈6.1 in the low-C band, as the majority of the stars in this metallicity range. Yet, constraining the isotopic ratio of key species, such as carbon, sheds light on the properties and origin of these elusive stars. Aims. We performed high-resolution observations of SMSS 1605−1443 with the ESPRESSO spectrograph to look for variations in the radial velocity ( v rad ) with time. These data have been combined with older MIKE and UVES archival observations to enlarge the temporal baseline. The 12 C/ 13 C isotopic ratio is also studied to explore the possibility of mass transfer from a binary companion. Methods. A cross-correlation function against a natural template was applied to detect v rad variability and a spectral synthesis technique was used to derive 12 C/ 13 C in the stellar atmosphere. Results. We confirm previous indications of binarity in SMSS 1605−1443 and measured a lower limit 12 C/ 13 C > 60 at more than a 3 σ confidence level, proving that this system is chemically unmixed and that no mass transfer from the unseen companion has happened so far. Thus, we confirm the CEMP-no nature of SMSS 1605−1443 and show that the pristine chemical composition of the cloud from which it formed is currently imprinted in its stellar atmosphere free of contamination." @default.
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- W4311454664 date "2023-01-01" @default.
- W4311454664 modified "2023-09-25" @default.
- W4311454664 title "The pristine nature of SMSS 1605−1443 revealed by ESPRESSO" @default.
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- W4311454664 doi "https://doi.org/10.1051/0004-6361/202245392" @default.
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