Research
see also Publications
Gaia - Taking the Galactic Census
Determination of Astrophysical Parameters for all stars observed by Gaia
Calibration of Astrophysical Parameters with models and observations of Benchmark stars
Supported by
VALD - an atomic and molecular database for astrophysics
M dwarfs
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Objective: Derive an improved metallicity scale for the lower main sequence.
Method: High resolution spectroscopy and abundance analysis of inactive M dwarfs.
Nearby stars
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Spectroscopy in the Local Neighborhood:
A High Resolution Survey and Abundance Analysis of Selected Stars
With R. Earle Luck
Publications:
Giants in the Local Region
Luck & Heiter (2007)
Dwarfs in the Local Region
Luck & Heiter (2006)
Stars within 15 Parsecs: Abundances for a Northern Sample
Luck & Heiter (2005)
Abundance Analysis of Planetary Host Stars. I. Differential Iron Abundances
Heiter & Luck (2003)
© 2016 Ulrike Heiter