Bridging model and observed stellar spectra

Bibcode
2011MNRAS.411..807A
DOI
10.1111/j.1365-2966.2010.17717.x
Allende-Prieto, C.
Bibliographical reference

Monthly Notices of the Royal Astronomical Society, Volume 411, Issue 2, pp. 807-812.

Advertised on:
2
2011
Journal
Monthly Notices of the Royal Astronomical Society
Number of authors
1
IAC number of authors
1
Citations
2
Refereed citations
2
Description
Accurate model stellar fluxes are key for the analysis of observations of individual stars or stellar populations. Model spectra differ from real stellar spectra due to limitations of the input physical data and adopted simplifications, but can be empirically calibrated to maximize their resemblance to actual stellar spectra. We describe a least-squares procedure of general use and test it on the MILES library.
Related projects
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)
Techniques
Galaxies

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