Abstract.
It is demonstrated that abundance patterns in extremely metal-deficient stars with [Mg/H] \(\lesssim\) -2 are remarkably similar to those seen in the individual first generation supernova remnants. This suggests that most of the stars with [Fe/H] \(\lesssim\) -2.5 were made from individual supernova events.
Author information
Authors and Affiliations
Editor information
Rights and permissions
About this paper
Cite this paper
Shigeyama, T., Tsujimoto, T. A New Model for Chemical Evolution in the Galactic Halo: First Stars with Heavy Elements. In: Weiss, A., Abel, T.G., Hill, V. (eds) The First Stars. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10719504_31
Download citation
DOI: https://doi.org/10.1007/10719504_31
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