Abstract
To study stellar populations, it is common to combine chemical abundances from different spectroscopic surveys/studies where different setups were used. These inhomogeneities can lead us to inaccurate scientific conclusions. In this work, we studied one aspect of the problem: When deriving chemical abundances from high-resolution stellar spectra, what differences originate from the use of different radiative transfer codes?
Original language | English |
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Title of host publication | Proceedings of the 12th Scientific Meeting of the Spanish Astronomical Society |
Subtitle of host publication | Highlights of Spanish Astrophysics IX, SEA 2016 |
Editors | S. Arribas, A. Alonso-Herrero, F. Figueras, C. Hernandez-Monteagudo, A. Sanchez-Lavega, S. Perez-Hoyos |
Place of Publication | Spain |
Publisher | Spanish Astronomical Society (SEA) |
Pages | 334-337 |
Number of pages | 4 |
ISBN (Electronic) | 9788461789313 |
Publication status | Published - 1 Jan 2016 |
Externally published | Yes |
Event | Scientific Meeting of the Spanish Astronomical Society: Highlights of Spanish Astrophysics IX - Bilbao, Spain Duration: 18 Jul 2016 → 22 Jul 2016 Conference number: 12th |
Conference
Conference | Scientific Meeting of the Spanish Astronomical Society |
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Abbreviated title | SEA 2016 |
Country/Territory | Spain |
City | Bilbao |
Period | 18/07/16 → 22/07/16 |