activity
20022019
most citedNew constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey

844 citations · 5.1k across the 47 of their papers we have counts for

collaborators

47 papers

astro-ph.SR2019★ 50 cited

The chemical composition of HIP34407/HIP34426 and other twin-star comoving pairs

I. Ramirez, S. Khanal, S. J. Lichon +4

We conducted a high-precision elemental abundance analysis of the twin-star comoving pair HIP34407/HIP34426. With mean error of 0.013 dex in the differential abundances (D[X/H]), a…

astro-ph.SR2019★ 65 cited

The Li-age correlation: the Sun is unusually Li deficient for its age

M. Carlos, J. Melendez, L. Spina +8

The present work aims to examine in detail the depletion of lithium in solar twins to better constrain stellar evolution models and investigate its possible connection with exoplan…

astro-ph.SR2018★ 36 cited

Detailed chemical compositions of the wide binary HD 80606/80607: revised stellar properties and constraints on planet formation

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

Differences in the elemental abundances of planet hosting stars in binary systems can give important clues and constraints about planet formation and evolution. In this study we pe…

astro-ph.SR2018★ 181 cited

The Chemical Homogeneity of Sun-like Stars in the Solar Neighborhood

Megan Bedell, Jacob L. Bean, Jorge Melendez +9

The compositions of stars are a critical diagnostic tool for many topics in astronomy such as the evolution of our Galaxy, the formation of planets, and the uniqueness of the Sun.…

astro-ph.SR2017★ 2 cited

iota Horologii is unlikely to be an evaporated Hyades star

I. Ramirez, D. Yong, E. Gutierrez +3

We present a high-precision chemical analysis of iota Horologii, a planet-host field star thought to have formed in the Hyades. Elements with atomic number 6<=Z<=30 have abundances…

astro-ph.SR2017★ 17 cited

On the Iron Abundance Anomaly in K-dwarf and Hyades Stars

Patrick D. Aleo, Alexander C. Sobotka, Ivan Ramirez

Using standard 1D-LTE model atmosphere analysis, we provide an in-depth investigation of iron abundance as derived from neutral and singly ionization iron lines (Fe {\scriptsize{I,…