How much can we trust high-resolution spectroscopic stellar chemical abundances?

S. Blanco-Cuaresma, T. Nordlander, U. Heiter, P. Jofré, T. Masseron, L. Casamiquela, H. M. Tabernero, S. S. Bhat, A. R. Casey, J. Meléndez, I. Ramírez

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

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.

Original languageEnglish
Title of host publicationProceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016
EditorsS. Arribas, A. Alonso-Herrero, F. Figueras, C. Hernandez-Monteagudo, A. Sanchez-Lavega, S. Perez-Hoyos
PublisherSEA
Pages334-337
Number of pages4
ISBN (Electronic)9788461789313
Publication statusPublished - 2016
Externally publishedYes
Event12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016 - Bilbao, Spain
Duration: 18 Jul 201622 Jul 2016

Publication series

NameProceedings of the 12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016

Conference

Conference12th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics IX, SEA 2016
Country/TerritorySpain
CityBilbao
Period18/07/1622/07/16

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