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Presupernova Evolution and Explosive Nucleosynthesis of Rotating Massive Stars in the Metallicity Range −3 ≤ [Fe/H] ≤ 0

The Astrophysical journal. Supplement series, 2018-07, Vol.237 (1), p.13

2018

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The Presupernova Core Mass-Radius Relation of Massive Stars: Understanding Its Formation and Evolution

The Astrophysical journal, 2020-02, Vol.890 (1), p.43

2020

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Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes

The Astrophysical journal, 2020-01, Vol.888 (2), p.76

2020

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Zero and Extremely Low-metallicity Rotating Massive Stars: Evolution, Explosion, and Nucleosynthesis Up to the Heaviest Nuclei

The Astrophysical journal. Supplement series, 2024-02, Vol.270 (2), p.28

2024

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Erratum: “Zero and Extremely Low-metallicity Rotating Massive Stars: Evolution, Explosion, and Nucleosynthesis Up to the Heaviest Nuclei” (2024, ApJS, 270, 28)

The Astrophysical journal. Supplement series, 2024-06, Vol.272 (2), p.48

2024

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Presupernova Evolution and Explosive Nucleosynthesis of Rotating Massive Stars. II. The Supersolar Models at [Fe/H] = 0.3

The Astrophysical journal. Supplement series, 2024-05, Vol.272 (1), p.15

2024

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Evolution and Final Fate of Solar Metallicity Stars in the Mass Range 7–15 M ⊙. I. The Transition from Asymptotic Giant Branch to Super-AGB Stars, Electron Capture, and Core-collapse Supernova Progenitors

The Astrophysical journal. Supplement series, 2024-02, Vol.270 (2), p.29

2024

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Explosion Mechanism of Core-collapse Supernovae: Role of the Si/Si–O Interface

The Astrophysical journal, 2023-05, Vol.949 (1), p.17

2023

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Seeding the second star – II. CEMP star formation enriched from faint supernovae

Monthly notices of the Royal Astronomical Society, 2020-09, Vol.497 (3), p.3149-3165

2020

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The formation of the extremely primitive star SDSS J102915+172927 relies on dust

Monthly notices of the Royal Astronomical Society. Letters, 2012-06, Vol.423 (1), p.L60-L64

2012

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Evolution, Explosion, and Nucleosynthesis of Core-Collapse Supernovae

The Astrophysical journal, 2003-07, Vol.592 (1), p.404-433

2003

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PRE-SUPERNOVA EVOLUTION OF ROTATING SOLAR METALLICITY STARS IN THE MASS RANGE 13-120 M ☉ AND THEIR EXPLOSIVE YIELDS

The Astrophysical journal, 2013-02, Vol.764 (1), p.21

2013

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Supernova dust formation and the grain growth in the early universe: the critical metallicity for low-mass star formation

Monthly notices of the Royal Astronomical Society, 2015-01, Vol.446 (3), p.2659-2659

2015

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Dust grain growth and the formation of the extremely primitive star SDSS J102915+172927

Monthly notices of the Royal Astronomical Society, 2014-04, Vol.439 (3), p.3121-3127

2014

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Impact of the New Measurement of the 12C + 12C Fusion Cross Section on the Final Compactness of Massive Stars

The Astrophysical journal, 2021-07, Vol.916 (2)

2021

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White paper on nuclear astrophysics and low energy nuclear physics Part 1: Nuclear astrophysics

Progress in particle and nuclear physics, 2017-05, Vol.94, p.1-67

2017

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The Synthesis of {sup 44}Ti and {sup 56}Ni in Massive Stars

The Astrophysical journal, 2017-02, Vol.836 (1)

2017

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Hydrodynamical Modeling of the Light Curves of Core-collapse Supernovae with HYPERION. I. The Mass Range 13-25 M , the Metallicities −3 ≤ [Fe/H] ≤ 0, and the Case of SN 1999em

The Astrophysical journal, 2020-10, Vol.902 (2), p.95

2020

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On the Origin of HE 0107–5240, the Most Iron-deficient Star Presently Known

The Astrophysical journal, 2003-09, Vol.594 (2), p.L123-L126

2003

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The Explosive Yields Produced by the First Generation of Core Collapse Supernovae and the Chemical Composition of Extremely Metal Poor Stars

The Astrophysical journal, 2002-09, Vol.577 (1), p.281-294

2002

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The Nucleosynthesis of (26)Al and (60)Fe in Solar Metallicity Stars Extending in Mass from 11 to 120 M( : The Hydrostatic and Explosive Contributions

The Astrophysical journal, 2006-08, Vol.647 (1), p.483-500

2006

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The Synthesis of 44Ti and 56Ni in Massive Stars

The Astrophysical journal, 2017-02, Vol.836 (1)

2017

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The Synthesis of 44 Ti and 56 Ni in Massive Stars

The Astrophysical journal, 2017-02, Vol.836 (1), p.79

2017

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Evolution and Nucleosynthesis of Zero-Metal Intermediate-Mass Stars

The Astrophysical journal, 2001-06, Vol.554 (2), p.1159-1174

2001

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Evolution and Nucleosynthesis in Low-Mass Asymptotic Giant Branch Stars. I. Formation of Population I Carbon Stars

The Astrophysical journal, 1997-03, Vol.478 (1), p.332-339

1997

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Presupernova Evolution and Explosive Nucleosynthesis of Rotating Massive Stars in the Metallicity Range −3 ≤ [Fe/H] ≤ 0

The Presupernova Core Mass-Radius Relation of Massive Stars: Understanding Its Formation and Evolution

Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes

Zero and Extremely Low-metallicity Rotating Massive Stars: Evolution, Explosion, and Nucleosynthesis Up to the Heaviest Nuclei

Erratum: “Zero and Extremely Low-metallicity Rotating Massive Stars: Evolution, Explosion, and Nucleosynthesis Up to the Heaviest Nuclei” (2024, ApJS, 270, 28)

Presupernova Evolution and Explosive Nucleosynthesis of Rotating Massive Stars. II. The Supersolar Models at [Fe/H] = 0.3

Evolution and Final Fate of Solar Metallicity Stars in the Mass Range 7–15 M ⊙. I. The Transition from Asymptotic Giant Branch to Super-AGB Stars, Electron Capture, and Core-collapse Supernova Progenitors

Explosion Mechanism of Core-collapse Supernovae: Role of the Si/Si–O Interface

Seeding the second star – II. CEMP star formation enriched from faint supernovae

The formation of the extremely primitive star SDSS J102915+172927 relies on dust

Evolution, Explosion, and Nucleosynthesis of Core-Collapse Supernovae

PRE-SUPERNOVA EVOLUTION OF ROTATING SOLAR METALLICITY STARS IN THE MASS RANGE 13-120 M ☉ AND THEIR EXPLOSIVE YIELDS

Supernova dust formation and the grain growth in the early universe: the critical metallicity for low-mass star formation

Dust grain growth and the formation of the extremely primitive star SDSS J102915+172927

Impact of the New Measurement of the 12C + 12C Fusion Cross Section on the Final Compactness of Massive Stars

White paper on nuclear astrophysics and low energy nuclear physics Part 1: Nuclear astrophysics

The Synthesis of {sup 44}Ti and {sup 56}Ni in Massive Stars

Hydrodynamical Modeling of the Light Curves of Core-collapse Supernovae with HYPERION. I. The Mass Range 13-25 M , the Metallicities −3 ≤ [Fe/H] ≤ 0, and the Case of SN 1999em

On the Origin of HE 0107–5240, the Most Iron-deficient Star Presently Known

The Explosive Yields Produced by the First Generation of Core Collapse Supernovae and the Chemical Composition of Extremely Metal Poor Stars

The Nucleosynthesis of (26)Al and (60)Fe in Solar Metallicity Stars Extending in Mass from 11 to 120 M( : The Hydrostatic and Explosive Contributions

The Synthesis of 44Ti and 56Ni in Massive Stars

The Synthesis of 44 Ti and 56 Ni in Massive Stars

Evolution and Nucleosynthesis of Zero-Metal Intermediate-Mass Stars

Evolution and Nucleosynthesis in Low-Mass Asymptotic Giant Branch Stars. I. Formation of Population I Carbon Stars

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