Correction to: sMILES SSPs: a library of semi-empirical MILES stellar population models with variable [α/Fe] abundances

Bibcode
2024MNRAS.534.4060K
DOI
10.1093/mnras/stae2368
Knowles, Adam T.; Sansom, A. E.; Vazdekis, A.; Allende Prieto, C.
Bibliographical reference

Monthly Notices of the Royal Astronomical Society

Advertised on:
11
2024
Journal
Monthly Notices of the Royal Astronomical Society
Number of authors
4
IAC number of authors
3
Citations
0
Refereed citations
0
Related projects
Group members
Traces of Galaxy Formation: Stellar populations, Dynamics and Morphology
We are a large, diverse, and very active research group aiming to provide a comprehensive picture for the formation of galaxies in the Universe. Rooted in detailed stellar population analysis, we are constantly exploring and developing new tools and ideas to understand how galaxies came to be what we now observe.
Anna
Ferré Mateu
In progress
spectrum of mercury lamp
Chemical Abundances in Stars
Stellar spectroscopy allows us to determine the properties and chemical compositions of stars. From this information for stars of different ages in the Milky Way, it is possible to reconstruct the chemical evolution of the Galaxy, as well as the origin of the elements heavier than boron, created mainly in stellar interiors. It is also possible to
Carlos
Allende Prieto
In progress
Type
Refereed
Stellar & Interstellar Physics (FEEI)

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