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

Autor
Gil Pons, P.; Doherty, C.; Gutierrez, J.; Siess, L.; Wattana, S.; Lau, H. B.; Lattanzio, J. C.
Tipus d'activitat
Article en revista
Revista
Publications of the Astronomical Society of Australia
Data de publicació
2018-11-29
Volum
35
DOI
https://doi.org/10.1017/pasa.2018.42 Obrir en finestra nova
Repositori
http://hdl.handle.net/2117/127718 Obrir en finestra nova
Resum
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...
Citació
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.
Paraules clau
Stars - AGB and post-AGB, Stars - Population III, Stars - abundances, Stars - evolution

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