activity
20162026
most citedThe Hyades open cluster is chemically inhomogeneous

95 citations · 231 across the 13 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR2026

The Sun's chemical peculiarity: disentangling Galactic chemical evolution and planetary engulfment in solar twins

Mia Babatsikos, Fan Liu, Amanda Karakas +5

Recent observational studies have suggested that the Sun may be chemically peculiar relative to the majority of solar twins. Here, we re-analyse high-resolution, high signal-to-noi…

astro-ph.SR2026

Planet engulfment in the chemically anomalous HD 129171/HD 129209 pair

Anne Rathsam, Jorge Meléndez, Rodolfo Smiljanic +2

Binary systems composed of stars with similar parameters should have identical chemical composition. However, many chemically anomalous pairs have been found in the literature, suc…

astro-ph.SR2025

C3PO V: Comoving stellar pairs indicate rotational spin-down drives the main-sequence Li-Dip

Qinghui Sun, Yuan-Sen Ting, Barbara J. Anthony-Twarog +4

The lithium-dip observed in mid-F dwarfs remains a long-standing challenge for stellar evolution models. We present high-precision stellar parameters and A(Li) for 22 new comoving…

astro-ph.SR2024

Planets Around Solar Twins/Analogs (PASTA) I.: High precision stellar chemical abundance for 17 planet-hosting stars and the condensation temperature trend

Qinghui Sun, Sharon Xuesong Wang, Tianjun Gan +30

The Sun is depleted in refractory elements compared to nearby solar twins, which may be linked to the formation of giant or terrestrial planets. Here we present high-resolution, hi…

astro-ph.SR2024★ 34 cited

At least one in a dozen stars exhibits evidence of planetary ingestion

Fan Liu, Yuan-Sen Ting, David Yong +6

Stellar chemical compositions can be altered by ingestion of planetary material and/or planet formation which removes refractory material from the proto-stellar disc. These "planet…

astro-ph.SR2021★ 30 cited

Detailed elemental abundances of binary stars: Searching for signatures of planet formation and atomic diffusion

Fan Liu, Bertram Bitsch, Martin Asplund +5

Binary star systems are assumed to be co-natal and coeval, thus to have identical chemical composition. In this work we aim to test the hypothesis that there is a connection betwee…

astro-ph.SR2019★ 68 cited

Chemical (in)homogeneity and atomic diffusion in the open cluster M67

F. Liu, M. Asplund, D. Yong +4

Context. The benchmark open cluster M67 is known to have solar metallicity and similar age as the Sun. It thus provides us a great opportunity to study the properties of solar twin…

astro-ph.SR2016★ 95 cited

The Hyades open cluster is chemically inhomogeneous

F. Liu, D. Yong, M. Asplund +2

We present a high-precision differential abundance analysis of 16 solar-type stars in the Hyades open cluster based on high resolution, high signal-to-noise ratio (S/N ~ 350 - 400)…