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Detailed chemical composition of classical Cepheids in the LMC cluster NGC 1866 and in the field of the SMC

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Cepheids are excellent tracers of young stellar populations. They play a crucial role in astrophysics as standard candles. The chemistry of classical Cepheids in the Milky Way is now quite well-known, however despite a much larger sample, the chemical composition of Magellanic Cepheids has been only...

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Bibliographic Details
Main Authors: Lemasle, Bertrand (Author) , Grebel, Eva K. (Author)
Format: Article (Journal)
Language:English
Published: 11 December 2017
In: Astronomy and astrophysics
Year: 2017, Volume: 608
ISSN:1432-0746
DOI:10.1051/0004-6361/201731370
Online Access:Verlag, kostenfrei, Volltext: http://dx.doi.org/10.1051/0004-6361/201731370
Verlag, kostenfrei, Volltext: https://www.aanda.org/articles/aa/abs/2017/12/aa31370-17/aa31370-17.html
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Author Notes:B. Lemasle, M.A.T. Groenewegen, E.K. Grebel, G. Bono, G. Fiorentino, P. François, L. Inno, V.V. Kovtyukh, N. Matsunaga, S. Pedicelli, F. Primas, J. Pritchard, M. Romaniello, and R. da Silva
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Detailed chemical composition of classical Cepheids in the LMC cluster NGC 1866 and in the field of the SMC by Lemasle, Bertrand (Author) , Grebel, Eva K. (Author) ,


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