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Sun-like stars unlike the Sun: Clues for chemical anomalies of cool stars
Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, P-4150762 Oporto, Portugal..
Univ Porto, Inst Astrofis & Ciencias Espaco, CAUP, Rua Estrelas, P-4150762 Oporto, Portugal..
Lund Observ, Dept Astron & Theoret Phys, Lund, Sweden..
Inst Astrofis Canarias, Tenerife, Spain.;Univ La Laguna, Dept Astrofis, Tenerife, Spain..
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2017 (English)In: Astronomical Notes - Astronomische Nachrichten, ISSN 0004-6337, E-ISSN 1521-3994, Vol. 338, no 4, 442-452 p.Article in journal (Refereed) Published
Abstract [en]

We present a summary of the splinter session Sun-like stars unlike the Sun that was held on June 9, 2016, as part of the Cool Stars 19 conference (Uppsala, Sweden), in which the main limitations (in the theory and observations) in the derivation of very precise stellar parameters and chemical abundances of Sun-like stars were discussed. The most important and most debated processes that can produce chemical peculiarities in solar-type stars were outlined and discussed. Finally, in an open discussion between all the participants, we tried to identify new pathways and prospects toward future solutions of the currently open questions.

Place, publisher, year, edition, pages
WILEY-V C H VERLAG GMBH , 2017. Vol. 338, no 4, 442-452 p.
Keyword [en]
stars: abundances, stars: chemically peculiar, (stars:) planetary systems, galaxy: abundances, (galaxy:) solar neighborhood
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:uu:diva-324615DOI: 10.1002/asna.201713315ISI: 000400944700008OAI: oai:DiVA.org:uu-324615DiVA: diva2:1110689
Available from: 2017-06-16 Created: 2017-06-16 Last updated: 2017-06-16Bibliographically approved

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Korn, Andreas J.Gustafsson, BengtLind, Karin
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CiteExportLink to record
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Citation style
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