CORDIS Project
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This project aims to identify and characterize extremely rare stars known as Population III stars, which are believed to have formed from metal-free clouds in the early universe. By utilizing advanced observational techniques and data analysis, the project seeks to enhance our understanding of the formation of the firs…
The number of identified primitive low-metallicity stars has steadily grown.
Today, we know of stars with less than one ten-millionth of the solar iron content, but no stars completely devoid of metals —known as Population III (Pop III)— have been identified so far.
It was commonly accepted that only massive, short-lived Pop III stars formed from metal-free clouds, but recent simulations suggest that their low-mass counterparts (<1M☉) could also form and may still survive today.
However, the mas…
INSTITUTO DE ASTROFISICA DE CANARIAS
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