Chemical evidence for planetary ingestion in a quarter of Sun-like stars-Reference-Cited by-同舟云学术

Chemical evidence for planetary ingestion in a quarter of Sun-like stars

Published:2021-08-30 Issue:11 Volume:5 Page:1163-1169
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Spina Lorenzo^ORCID,Sharma Parth,Meléndez Jorge^ORCID,Bedell Megan^ORCID,Casey Andrew R.^ORCID,Carlos Marília^ORCID,Franciosini Elena^ORCID,Vallenari Antonella^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

https://www.nature.com/articles/s41550-021-01451-8.pdf

Reference51 articles.

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3. Pinsonneault, M. H., DePoy, D. L. & Coffee, M. The mass of the convective zone in FGK main-sequence stars and the effect of accreted planetary material on apparent metallicity determinations. Astrophys. J. Lett. 556, L59–L62 (2001).

4. Cowley, C. R., Bord, D. J. & Yüce, K. Modeling stellar abundance patterns resulting from the addition of earth-like planetary material. Astron. J. 161, 142 (2021).

5. Chambers, J. E. Stellar elemental abundance patterns: implications for planet formation. Astrophys. J. 724, 92–97 (2010).

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