Detailed abundances of planet-hosting wide binaries. I. Did planet formation imprint chemical signatures in the atmospheres of HD 20782/81?
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Mack III, Claude
Schuler, Simon
Stassun, Keivan
Norris, John
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IOP Publishing
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Using high-resolution, high signal-to-noise echelle spectra obtained with Magellan/MIKE, we present a detailed chemical abundance analysis of both stars in the planet-hosting wide binary system HD 20782 + HD 20781. Both stars are G dwarfs, and presumably
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Astrophysical Journal, The
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Open Access
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