activity
20082023
most citedThe peculiar solar composition and its possible relation to planet formation

456 citations · 2.5k across the 30 of their papers we have counts for

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Showing astro-ph.SRShow all

20 papers · 1 filter

astro-ph.SR2023

C3PO: Towards a complete census of co-moving pairs of stars. I. High precision stellar parameters for 250 stars

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

We conduct a line-by-line differential analysis of a sample of 125 co-moving pairs of stars (dwarfs and subgiants near solar metallicity). We obtain high precision stellar paramete…

astro-ph.SR2020★ 10 cited

Constraining Nucleosynthesis in Two CEMP Progenitors Using Fluorine

A. Mura-Guzmán, D. Yong, C. Abate +6

We present new fluorine abundance estimations in two carbon enhanced metal-poor (CEMP) stars, HE 1429-0551 and HE 1305+0007. HE 1429-0551 is also enriched in slow neutron-capture p…

astro-ph.SR2020★ 44 cited

Detailed chemical compositions of planet hosting stars: I. Exploration of possible planet signatures

F. Liu, D. Yong, M. Asplund +5

We present a line-by-line differential analysis of a sample of 16 planet hosting stars and 68 comparison stars using high resolution, high signal-to-noise ratio spectra gathered us…

astro-ph.SR2019★ 43 cited

Chemical abundances along the 1G sequence of the chromosome maps: The Globular Cluster NGC 3201

A. F. Marino, A. P. Milone, A. Sills +10

The Hubble Space Telescope (HST) UV Legacy Survey of Galactic Globular Clusters (GCs) has investigated multiple stellar populations by means of the "chromosome map" (ChM) diagnosti…

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.SR2019★ 13 cited

An investigation of C, N and Na abundances in red giant stars of the Sculptor dwarf spheroidal galaxy

C. Salgado, G. S. Da Costa, J. E. Norris +1

The origin of the star-to-star abundance variations found for the light elements in Galactic globular clusters (GGCs) is not well understood, which is a significant problem for ste…