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

QB460-466 Earth and Planetary Astrophysics (astro-ph.EP) Exoplanet formation Solar analogs Astrophysics - Solar and Stellar Astrophysics FOS: Physical sciences Planet hosting stars Astrophysics Solar and Stellar Astrophysics (astro-ph.SR) Stellar abundances Astrophysics - Earth and Planetary Astrophysics
DOI: 10.48550/arxiv.2411.13825 Publication Date: 2024-11-20
ABSTRACT
The Sun is depleted in refractory elements compared to nearby solar twins, which may be linked the formation of giant or terrestrial planets. Here we present high-resolution, high signal-to-noise spectroscopic data for 17 solar-like stars hosting planets, obtained with Magellan II/MIKE, investigate whether this depletion related planet formation. We derive stellar parameters, including atmosphere, age, radius, mass, and chemical abundances 22 from carbon europium through line-by-line differential analysis. Our uncertainties range 0.01 dex Fe Si 0.08 Sr, Y, Eu. By comparing those stars, abundance ([X/Fe]$_{\rm solar}$ - [X/Fe]$_{\rm star}$) versus condensation temperature ($T_c$) trend. In particular, apply Galactic evolution corrections five twins within full sample. results conform previous studies that relatively volatile elements. For both rest find all known gas planets exhibit negative $T_c$ trend slopes, suggesting similar giant-planet-host stars. Additionally, no correlation between slopes total mass detected each system, not cause element Sun.
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