Infrared Laboratory Oscillator Strengths of Fe I in the H-band

Bibcode
2013ApJ...779...17R
DOI
10.1088/0004-637X/779/1/17
Ruffoni, M. P.; Allende Prieto, C.; Nave, G.; Pickering, J. C.
Bibliographical reference

The Astrophysical Journal, Volume 779, Issue 1, article id. 17, 8 pp. (2013).

Advertised on:
12
2013
Journal
The Astrophysical Journal
Number of authors
4
IAC number of authors
1
Citations
22
Refereed citations
19
Description
We report experimental oscillator strengths for 28 infrared Fe I transitions, for which no previous experimental values exist. These transitions were selected to address an urgent need for oscillator strengths of lines in the H-band (between 1.4 μm and 1.7 μm) required for the analysis of spectra obtained from the Sloan Digital Sky Survey (SDSS-III) Apache Point Galactic Evolution Experiment (APOGEE). Upper limits have been placed on the oscillator strengths of an additional seven transitions, predicted to be significant by published semi-empirical calculations, but not observed to be so.
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)
Methods
Techniques

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