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Sun-like stars unlike the Sun : Clues for chemical anomaliesof cool stars

Adibekyan, V. ; Delgado-Mena, E. ; Feltzing, S. LU orcid ; González Hernández, J. I. ; Hinkel, Natalie R. ; Korn, A. J. ; Asplund, M. ; Beck, P. G. ; Deal, M. and Gustafsson, B. , et al. (2017) In Astronomical Notes - Astronomische Nachrichten 338(4). p.442-452
Abstract

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.

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organization
publishing date
type
Contribution to journal
publication status
published
subject
keywords
(galaxy:) solar neighborhood, (stars:) planetary systems, galaxy: abundances, stars: abundances, stars: chemically peculiar
in
Astronomical Notes - Astronomische Nachrichten
volume
338
issue
4
pages
11 pages
publisher
John Wiley & Sons Inc.
external identifiers
  • wos:000400944700008
  • scopus:85018376187
ISSN
0004-6337
DOI
10.1002/asna.201713315
language
English
LU publication?
yes
id
4edad18f-6ce9-45dd-ad97-ebf2f6ebf215
date added to LUP
2017-05-18 09:17:21
date last changed
2025-01-07 13:40:10
@article{4edad18f-6ce9-45dd-ad97-ebf2f6ebf215,
  abstract     = {{<p>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.</p>}},
  author       = {{Adibekyan, V. and Delgado-Mena, E. and Feltzing, S. and González Hernández, J. I. and Hinkel, Natalie R. and Korn, A. J. and Asplund, M. and Beck, P. G. and Deal, M. and Gustafsson, B. and Honda, S. and Lind, K and Nissen, P. E. and Spina, L.}},
  issn         = {{0004-6337}},
  keywords     = {{(galaxy:) solar neighborhood; (stars:) planetary systems; galaxy: abundances; stars: abundances; stars: chemically peculiar}},
  language     = {{eng}},
  month        = {{05}},
  number       = {{4}},
  pages        = {{442--452}},
  publisher    = {{John Wiley & Sons Inc.}},
  series       = {{Astronomical Notes - Astronomische Nachrichten}},
  title        = {{Sun-like stars unlike the Sun : Clues for chemical anomaliesof cool stars}},
  url          = {{http://dx.doi.org/10.1002/asna.201713315}},
  doi          = {{10.1002/asna.201713315}},
  volume       = {{338}},
  year         = {{2017}},
}