Zero and Extremely Low-metallicity Rotating Massive Stars: Evolution, Explosion, and Nucleosynthesis Up to the Heaviest Nuclei
We present the evolution and the explosion of two massive stars, 15 and 25 M _⊙ , spanning a wide range of initial rotation velocities (from 0 to 800 km s ^−1 ) and three initial metallicities: Z = 0 ([Fe/H] = −∞), 3.236 × 10 ^−7 ([Fe/H] = −5), and 3.236 × 10 ^−6 ([Fe/H] = −4). A very large nuclear...
Main Authors: | , , |
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Format: | Article |
Language: | English |
Published: |
IOP Publishing
2024-01-01
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Series: | The Astrophysical Journal Supplement Series |
Subjects: | |
Online Access: | https://doi.org/10.3847/1538-4365/ad1686 |