ESA Data Ontology: ESADO: Population III stars

Stellar astronomy > Stellar populations > Population III stars

Population III stars

A member of the first generation of stars, formed out of pristine gas, enriched by primordial nucleosynthesis alone. The material from which these stars formed consisted mostly of hydrogen and helium. Because neutral hydrogen clouds were free of dust, their cooling mechanism was drastically ineffective. As a result, these star forming clouds had a much higher temperature than in the present epoch, and their Jeans mass was much higher. Therefore, these first generation of stars were principally massive, with a typical mass scale of order of about 100 M_sun. Population III stars started forming about 300 million years after the Big Bang at redshifts between 50 and 6, when the Universe had between 1 and 5% of its present age. These stars were probably responsible for the reionization of the Universe. Given their high mass, they lived only a few million years ending with either a pair-instability supernova phase or a direct collapse to a black hole. Population III stars thus initiated the chemical enrichment of the Universe and opened the way to more normal modes of star formation, namely Population II. Some models predict a bimodal initial mass function for the first stars, allowing also for solar mass stars. (en)

Hypothetical population of extremely massive and hot stars with virtually no metals. (en)

http://astrothesaurus.org/uat/1285

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