Abstract.
In this paper, first we summarize the many reasons that over the years led to introduce the concept of Pop-III stars. Second, we shortly cast the problem of their mass-scale and initial mass function. Third, we highlight the distinct behavior of zero-metal stars with respect to those of normal and low metal content, and concisely discuss their inner structure and path on the HR diagram in the mass range 0.9 to 100 M\(_\odot\) limited to core H- and He-burnings. Finally, we draw some general remarks on the stellar ejecta as a function of the chemical composition, and present some preliminary results concerning the ejecta from massive Pop-III stars due to stellar winds during the early stages.
Preview
Unable to display preview. Download preview PDF.
Author information
Authors and Affiliations
Editor information
Rights and permissions
About this paper
Cite this paper
Chiosi, C. Evolution of Pop III Stars. In: Weiss, A., Abel, T.G., Hill, V. (eds) The First Stars. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10719504_16
Download citation
DOI: https://doi.org/10.1007/10719504_16
Published:
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-67222-7
Online ISBN: 978-3-540-46461-7
eBook Packages: Springer Book Archive