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Primordial to extremely metal-poor AGB and Super-AGB stars: White dwarf or supernova progenitors?

Author
Gil Pons, P.; Doherty, C.; Gutierrez, J.; Siess, L.; Wattana, S.; Lau, H. B.; Lattanzio, J. C.
Type of activity
Journal article
Journal
Publications of the Astronomical Society of Australia
Date of publication
2018-11-29
Volume
35
DOI
https://doi.org/10.1017/pasa.2018.42 Open in new window
Repository
http://hdl.handle.net/2117/127718 Open in new window
Abstract
Getting a better understanding of the evolution and nucleosynthetic yields of the most metal-poor stars ( Z ¿ 10 ¿5 ) is critical because they are part of the big picture of the history of the primitive universe. Yet many of the remaining unknowns of stellar evolution lie in the birth, life, and death of these objects. We review stellar evolution of intermediate-mass Z = 10 ¿5 models existing in the literature, with a particular focus on the problem of their final fates. We emphasise the impo...
Citation
Gil Pons, P. [et al.]. Primordial to extremely metal-poor AGB and Super-AGB stars: White dwarf or supernova progenitors?. "Publications of the Astronomical Society of Australia", 29 Novembre 2018, vol. 35.
Keywords
Stars - AGB and post-AGB, Stars - Population III, Stars - abundances, Stars - evolution

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