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Very low-metallicity massive stars : Pre-SN evolution models and primary nitrogen production

Astronomy and astrophysics (Berlin), 2007, Vol.461 (2), p.571-583

HIRSCHI, R

2007

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The role of neutron star mergers in the chemical evolution of the Galactic halo

Astronomy and astrophysics (Berlin), 2015-05, Vol.577, p.A139

2015

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Evolution of Wolf–Rayet stars as black hole progenitors

Monthly notices of the Royal Astronomical Society, 2021-08, Vol.505 (4), p.4874-4889

2021

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NuGrid stellar data set – II. Stellar yields from H to Bi for stellar models with MZAMS = 1–25 M⊙ and Z = 0.0001–0.02

Monthly notices of the Royal Astronomical Society, 2018-10, Vol.480 (1), p.538-571

2018

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Dependence of convective boundary mixing on boundary properties and turbulence strength

Monthly notices of the Royal Astronomical Society, 2019-04, Vol.484 (4), p.4645-4664

2019

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3D hydrodynamic simulations of carbon burning in massive stars

Monthly notices of the Royal Astronomical Society, 2017-10, Vol.471 (1), p.279-300

2017

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The contribution from rotating massive stars to the enrichment in Sr and Ba of the Milky Way

Monthly notices of the Royal Astronomical Society, 2019-09, Vol.489 (4), p.5244-5255

2019

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The s-process in the Galactic halo: the fifth signature of spinstars in the early Universe?

Astronomy and astrophysics (Berlin), 2013-05, Vol.553, p.1-13

2013

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NUGRID STELLAR DATA SET. I. STELLAR YIELDS FROM H TO BI FOR STARS WITH METALLICITIES Z = 0.02 and Z = 0.01

The Astrophysical journal. Supplement series, 2016-08, Vol.225 (2), p.24-24

2016

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Uncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations

Monthly notices of the Royal Astronomical Society, 2018-03, Vol.474 (3), p.3133-3139

2018

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Grids of stellar models with rotation: II. WR populations and supernovae/GRB progenitors at Z = 0.014

Astronomy and astrophysics (Berlin), 2012-06, Vol.542, p.A29

2012

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Non-standard s-process in low metallicity massive rotating stars

Astronomy and astrophysics (Berlin), 2012-02, Vol.538, p.L2

2012

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Effects of rotation on the evolution of primordial stars

Astronomy and astrophysics (Berlin), 2008-10, Vol.489 (2), p.685-698

2008

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Nucleosynthesis in early rotating massive stars and chemical composition of CEMP stars

Journal of physics. Conference series, 2020-10, Vol.1668 (1), p.12006

2020

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Convective core entrainment in 1D main-sequence stellar models

Monthly notices of the Royal Astronomical Society, 2021-05, Vol.503 (3), p.4208-4220

2021

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Uncertainties in the production of p nuclei in massive stars obtained from Monte Carlo variations

Monthly notices of the Royal Astronomical Society, 2016-12, Vol.463 (4), p.4153-4153

2016

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The Nuclear Reaction Network WinNet

The Astrophysical journal. Supplement series, 2023-10, Vol.268 (2), p.66

2023

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Multidimensional low-Mach number time-implicit hydrodynamic simulations of convective helium shell burning in a massive star

Astronomy and astrophysics (Berlin), 2021-09, Vol.653, p.A55

2021

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Constraining the efficiency of angular momentum transport with asteroseismology of red giants: the effect of stellar mass

Astronomy and astrophysics (Berlin), 2017-03, Vol.599, p.A18

2017

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NuGrid stellar data set – III. Updated low-mass AGB models and s-process nucleosynthesis with metallicities Z= 0.01, Z = 0.02, and Z = 0.03

Monthly notices of the Royal Astronomical Society, 2019-10, Vol.489 (1), p.1082-1098

2019

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APPLICATION OF A THEORY AND SIMULATION-BASED CONVECTIVE BOUNDARY MIXING MODEL FOR AGB STAR EVOLUTION AND NUCLEOSYNTHESIS

The Astrophysical journal, 2016-08, Vol.827 (1), p.30-30

2016

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Constraints on stellar rotation from the evolution of Sr and Ba in the Galactic halo

Monthly notices of the Royal Astronomical Society, 2021-04, Vol.502 (2), p.2495-2507

2021

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Are C-rich ultra iron-poor stars also He-rich?

Astronomy and astrophysics (Berlin), 2010-10, Vol.521, p.A30

2010

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3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star

Monthly notices of the Royal Astronomical Society, 2023-05, Vol.523 (2), p.2317-2328

2023

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Uncertainties in νp-process nucleosynthesis from Monte Carlo variation of reaction rates

Monthly notices of the Royal Astronomical Society, 2019-10, Vol.489 (1), p.1379-1396

2019

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Very low-metallicity massive stars : Pre-SN evolution models and primary nitrogen production

The role of neutron star mergers in the chemical evolution of the Galactic halo

Evolution of Wolf–Rayet stars as black hole progenitors

NuGrid stellar data set – II. Stellar yields from H to Bi for stellar models with MZAMS = 1–25 M⊙ and Z = 0.0001–0.02

Dependence of convective boundary mixing on boundary properties and turbulence strength

3D hydrodynamic simulations of carbon burning in massive stars

The contribution from rotating massive stars to the enrichment in Sr and Ba of the Milky Way

The s-process in the Galactic halo: the fifth signature of spinstars in the early Universe?

NUGRID STELLAR DATA SET. I. STELLAR YIELDS FROM H TO BI FOR STARS WITH METALLICITIES Z = 0.02 and Z = 0.01

Uncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations

Grids of stellar models with rotation: II. WR populations and supernovae/GRB progenitors at Z = 0.014

Non-standard s-process in low metallicity massive rotating stars

Effects of rotation on the evolution of primordial stars

Nucleosynthesis in early rotating massive stars and chemical composition of CEMP stars

Convective core entrainment in 1D main-sequence stellar models

Uncertainties in the production of p nuclei in massive stars obtained from Monte Carlo variations

The Nuclear Reaction Network WinNet

Multidimensional low-Mach number time-implicit hydrodynamic simulations of convective helium shell burning in a massive star

Constraining the efficiency of angular momentum transport with asteroseismology of red giants: the effect of stellar mass

NuGrid stellar data set – III. Updated low-mass AGB models and s-process nucleosynthesis with metallicities Z= 0.01, Z = 0.02, and Z = 0.03

APPLICATION OF A THEORY AND SIMULATION-BASED CONVECTIVE BOUNDARY MIXING MODEL FOR AGB STAR EVOLUTION AND NUCLEOSYNTHESIS

Constraints on stellar rotation from the evolution of Sr and Ba in the Galactic halo

Are C-rich ultra iron-poor stars also He-rich?

3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star

Uncertainties in νp-process nucleosynthesis from Monte Carlo variation of reaction rates

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