UBC 1052 is a 2.25 Gyr old inner-disc open cluster at Z=340 pc with [Fe/H]=0.05 dex and unique abundance patterns among high-resolution studied clusters, consistent with inward migration.
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3 Pith papers cite this work. Polarity classification is still indexing.
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Derives homogeneous n-capture element abundances for GBSv3 sample via iSpec spectral analysis and clustering for line selection, yielding measurements in agreement with literature.
High-precision abundances and Ba isotopic ratios in TYC 6044-714-1 favor an s+r nucleosynthesis scenario over i-process models, which require implausible conditions and mismatch isotopic data.
citing papers explorer
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The high-altitude, inner-disc, and chemically peculiar open cluster UBC 1052
UBC 1052 is a 2.25 Gyr old inner-disc open cluster at Z=340 pc with [Fe/H]=0.05 dex and unique abundance patterns among high-resolution studied clusters, consistent with inward migration.
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Gaia FGK benchmark stars: abundances of \textit{n}-capture elements of the third version
Derives homogeneous n-capture element abundances for GBSv3 sample via iSpec spectral analysis and clustering for line selection, yielding measurements in agreement with literature.
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Observational Signatures and Constraints on the Intermediate Neutron-Capture Process. The Case of the CEMP star TYC 6044-714-1 (RAVE J094921.8-161722)
High-precision abundances and Ba isotopic ratios in TYC 6044-714-1 favor an s+r nucleosynthesis scenario over i-process models, which require implausible conditions and mismatch isotopic data.