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Kronos and Krios: Evidence for Accretion of a Massive, Rocky Planetary System in a Comoving Pair of Solar-type Stars

  • Authors: Semyeong Oh, Adrian M. Price-Whelan, John M. Brewer, David W. Hogg, David N. Spergel, and Justin Myles

2018 The Astrophysical Journal 854 138.

  • Provider: AAS Journals

Caption: Figure 2.

Abundances of the comoving pair Krios (blue) and Kronos (red). Lines are drawn for each star only to guide the eye. Kronos is enhanced in ﹩\mathrm{Fe}﹩ by ≈0.2 dex relative to Krios along with ﹩\mathrm{Mg}﹩, ﹩\mathrm{Al}﹩, ﹩\mathrm{Si}﹩, ﹩\mathrm{Ca}﹩, ﹩\mathrm{Ti}﹩, ﹩{\rm{V}}﹩, ﹩\mathrm{Cr}﹩, ﹩\mathrm{Ni}﹩, and ﹩{\rm{Y}}﹩, but not in ﹩{\rm{C}}﹩, ﹩{\rm{N}}﹩, ﹩{\rm{O}}﹩, ﹩\mathrm{Na}﹩, and ﹩\mathrm{Mn}﹩.

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