Publications (72)
Complete nucleosynthesis calculations for low-mass stars from NuGrid
Marco Pignatari, Falk Herwig, Michael Bennett +8
Mass loss and very low-metallicity stars
Raphael Hirschi, Cristina Chiappini, Georges Meynet +2
A chemical signature from fast-rotating low-metallicity massive stars: ROA 276 in omega Centauri
David Yong, John E. Norris, Gary S. Da Costa +5
Possible pair-instability supernovae at solar metallicity from magnetic stellar progenitors
Cyril Georgy, Georges Meynet, Sylvia Ekström +4
The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 Msun stellar mass limit
Paul A Crowther, Olivier Schnurr, Raphael Hirschi +4
PopII 1/2 stars: very high N14 and low O16 yields
Raphael Hirschi
The s-Process Enrichment of the Globular Clusters M4 and M22
Luke J. Shingles, Amanda I. Karakas, Raphael Hirschi +4
Nucleosynthesis simulations for a wide range of nuclear production sites from NuGrid
Falk Herwig, Michael Bennett, Steven Diehl +8
The impact of reduced mass loss rates on the evolution of massive stars
Raphael Hirschi
Pre-supernova mixing in CEMP-no source stars
Arthur Choplin, Sylvia Ekström, Georges Meynet +3
Nucleosynthesis Calculations from Core-Collapse Supernovae
Christopher L. Fryer, Patrick Young, Michael Bennett +8
OGLE14-073 - a promising pair-instability supernova candidate
Alexandra Kozyreva, Markus Kromer, Ulrich M. Noebauer +1
Origin of CEMP stars: What helium and lithium can tell us about CEMP stars?
Georges Meynet, Raphael Hirschi, Sylvia Ekstrom +4
Evolution and Nucleosynthesis of Very Massive Stars
Raphael Hirschi
Developments in physics of massive stars
Georges Meynet, Sylvia Ekstrom, Andre Maeder +3
Linking 1D Stellar Evolution to 3D Hydrodynamical Simulations
Andrea Cristini, Raphael Hirschi, Cyril Georgy +3
Constraints on rotational mixing from surface evolution of light elements in massive stars
Urs Frischknecht, Raphael Hirschi, Georges Meynet +5
Evolution and fate of very massive stars
Norhasliza Yusof, Raphael Hirschi, Georges Meynet +6
Rotating massive stars @ very low Z: high C and N production
Raphael Hirschi
Massive Stars as Cosmic Engines through the Ages
Andre Maeder, Georges Meynet, Sylvia Ekstrom +2
Uncertainties in s-process nucleosynthesis in massive stars determined by Monte Carlo variations
Nobuya Nishimura, Raphael Hirschi, Thomas Rauscher +2
Effects of Rotation on Presupernovae Models
Georges Meynet, Raphael Hirschi, André Maeder
NuGrid: Toward High Precision Double-Degenerate Merger Simulations with SPH in 3D
Steven Diehl, Christopher L. Fryer, Aimee Hungerford +11
Are some CEMP-s stars the daughters of spinstars?
Arthur Choplin, Raphael Hirschi, Georges Meynet +1
Grids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)
Sylvia Ekström, Cyril Georgy, Patrick Eggenberger +9
Spatial Distribution of Nucleosynthesis Products in Cassiopeia A: Comparison Between Observations and 3D Explosion Models
Patrick Young, Carola I. Ellinger, Francis X. Timmes +10
Are C-rich ultra iron poor stars also He-rich?
Georges Meynet, Raphael Hirschi, Sylvia Ekstrom +4
Evolution and chemical and dynamical effects of high-mass stars
Georges Meynet, Cristina Chiappini, Cyril Georgy +4
Progenitors of Core-Collapse Supernovae
Raphael Hirschi, David Arnett, Andrea Cristini +3
Massive Star Evolution: What we do (not) know
Cyril Georgy, Raphael Hirschi, Sylvia Ekström
The oldest stars of the bulge: new information on the ancient Galaxy
Gabriele Cescutti, Cristina Chiappini, Raphael Hirschi
Stellar Evolution Constraints on the Triple-Alpha Reaction Rate
Takuma Suda, Raphael Hirschi, Masayuki Y. Fujimoto
The evolution of massive stars in the context of V838 Monocerotis
Raphael Hirschi
Nucleosynthesis in Rotating massive stars and Abundances in the Early Galaxy
Georges Meynet, Raphael Hirschi, Sylvia Ekstrom +4
Linking 1D Evolutionary to 3D Hydrodynamical Simulations of Massive Stars
Andréa Cristini, Casey Meakin, Raphael Hirschi +3
The s-process in the Galactic halo: the fifth signature of spinstars in the early Universe?
Gabriele Cescutti, Cristina Chiappini, Raphael Hirschi +2
Grids of stellar models with rotation II. WR populations and supernovae/GRB progenitors at Z = 0.014
Cyril Georgy, Sylvia Ekström, Georges Meynet +5
Massive Stars and their Supernovae
Friedrich-Karl Thielemann, Raphael Hirschi, Matthias Liebendörfer +1
Grids of stellar models with rotation - III. Models from 0.8 to 120 Msun at a metallicity Z = 0.002
Cyril Georgy, Sylvia Ekström, Patrick Eggenberger +11
Testing a one-dimensional prescription of dynamical shear mixing with a two-dimensional hydrodynamic simulation
Philipp V. F. Edelmann, Friedrich K. Roepke, Raphael Hirschi +2
$s$-process production in rotating massive stars at solar and low metallicities
Urs Frischknecht, Raphael Hirschi, Marco Pignatari +7
Mass loss of rotating stars at very low metallicity
Georges Meynet, Andre Maeder, Raphael Hirschi +2
Advanced burning stages and fate of 8-10 Mo stars
Samuel Jones, Raphael Hirschi, Ken'ichi Nomoto +9
Pair-Instability Supernova Simulations: Progenitor Evolution, Explosion, and Light Curves
Matthew S. Gilmer, Alexandra Kozyreva, Raphael Hirschi +2
Convective-reactive proton-C12 combustion in Sakurai's object (V4334 Sagittarii) and implications for the evolution and yields from the first generations of stars
Falk Herwig, Marco Pignatari, Paul R. Woodward +5
Stellar yields in CNO from rotating stellar models
Georges Meynet, Andre Maeder, Raphael Hirschi
Nucleosynthesis in the first massive stars
Arthur Choplin, Georges Meynet, Andre Maeder +2
Evolution of rotating stars at very low metallicity
Georges Meynet, Raphael Hirschi, Sylvia Ekstrom +1
Evolution of the Most Massive Stars
André Maeder, Georges Meynet, Raphael Hirschi
Red Supergiants, Luminous Blue Variables and Wolf-Rayet stars: the single massive star perspective
Georges Meynet, Cyril Georgy, Raphael Hirschi +4
Life and Death of Very Massive Stars
Norhasliza Yusof, Hasan Abu Kassima, Raphael Hirschi +4
How much radioactive nickel does ASASSN-15lh require?
Alexandra Kozyreva, Raphael Hirschi, Sergey Blinnikov +1
Massive star evolution: from the early to the present day Universe
Georges Meynet, Sylvia Ekstrom, Cyril Georgy +2
The final fate of stars that ignite neon and oxygen off-center: electron capture or iron core-collapse supernova?
Samuel Jones, Raphael Hirschi, Ken'ichi Nomoto
The GSF Instability and Turbulence do not Account for the Relatively Low Rotation Rate of Pulsars
Raphael Hirschi, André Maeder
Pair-Instability Supernovae in the Local Universe
Daniel J. Whalen, Wesley Even, Joseph Smidt +7
Dynamical shear instability
Raphael Hirschi, Andre Maeder, Georges Meynet
44Ti and 56Ni in core-collapse supernovae
Georgios Magkotsios, Francis X. Timmes, Michael Wiescher +9
Wolf-Rayet stars as an evolved stage of stellar life
Cyril Georgy, Sylvia Ekström, Raphael Hirschi +3
Difficulties in Probing Nuclear Physics: A Study of $^{44}$Ti and $^{56}$Ni
Aimee Hungerford, Christopher L. Fryer, Francis X. Timmes +8
Fast evolving pair-instability supernova models: evolution, explosion, light curves
Alexandra Kozyreva, Matthew Gilmer, Raphael Hirschi +11
Chemical Abundances and Yields from Massive Stars
André Maeder, Georges Meynet, Raphael Hirschi
Effects of Dimensionality on Pair-Instability Supernova Explosions
Matthew S. Gilmer, Alexandra Kozyreva, Raphael Hirschi +1
Pre-suprenova evolution of rotating massive stars
Raphael Hirschi, Georges Meynet, Andre Maeder +1
3D Hydrodynamic Simulations of Carbon Burning in Massive Stars
Andrea Cristini, Casey Meakin, Raphael Hirschi +3
Very low metallicity massive star models: Pre-SN evolution and primary nitrogen production
Raphael Hirschi
Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning
Samuel Jones, Raphael Hirschi, Marco Pignatari +5
The First 3D Simulations of Carbon Burning in a Massive Star
Andrea Cristini, Casey Meakin, Raphael Hirschi +3
Nucleosynthetic Yields from "Collapsars"
Gabriel Rockefeller, Christopher L. Fryer, Patrick Young +8
NuGrid: s process in massive stars
Raphael Hirschi, Urs Frischknecht, F. -K. Thielemann +10
Non standard s-process in massive rotating stars. Yields of $10-150$ $M_{\odot}$ models at $Z=10^{-3}$
Arthur Choplin, Raphael Hirschi, Georges Meynet +3
The effect of 12C + 12C rate uncertainties on the weak s-process component
Michael E. Bennett, Raphael Hirschi, Marco Pignatari +9