CORDIS Project
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This research combines advanced spectroscopy and laser techniques to analyze infrared stellar objects. It aims to measure atomic transition lines to derive key atmospheric parameters like temperature and metallicity, enhancing our understanding of these celestial bodies.
This proposal combines state-of-the-art laboratory atomic spectroscopy and laser physics to provide a new and better understanding of infrared astrophysical objects.
The aim of the research is to use radiative lifetimes in combination with branching fractions (BF) to obtain oscillator strengths for atomic transition lines.
Specific 'tracer' lines will be used to determine, often for the first time, accurate effective temperature, metallicity, and surface gravity, for IR stellar objects including…
MAX IV Laboratory, Lund University
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