Selected:
Stellar Evolution Theory (Project)
Description: No description
SEEK ID: https://publications.h-its.org/projects/18
Description: No description
SEEK ID: https://publications.h-its.org/projects/18
- Stellar Evolution Theory
- The MiMeS survey of magnetism in massive stars: magnetic properties of the O-type star population
- A census of massive stars in NGC 346. Stellar parameters and rotational velocities
- Hydrodynamical simulations and similarity relations for eruptive mass-loss from massive stars
- The VLT-FLAMES Tarantula Survey. XXX. Red stragglers in the clusters Hodge 301 and SL 639
- Stellar mergers as the origin of magnetic massive stars
- Pre-supernova evolution, compact-object masses, and explosion properties of stripped binary stars
- The R136 star cluster dissected with Hubble Space Telescope/STIS - II. Physical properties of the most massive stars in R136
- Common-envelope evolution with an asymptotic giant branch star
- Formation of sdB-stars via common envelope ejection by substellar companions
- The VLT-FLAMES Tarantula Survey
- The Art of Modeling Stellar Mergers and the Case of the B[e] Supergiant R4 in the Small Magellanic Cloud
- Long-term evolution of a magnetic massive merger product
- Properties of OB star-black hole systems derived from detailed binary evolution models
- The Tarantula Massive Binary Monitoring. IV. Double-lined photometric binaries
- The Tarantula Massive Binary Monitoring. III. Atmosphere analysis of double-lined spectroscopic systems
- The young massive SMC cluster NGC 330 seen by MUSE. I. Observations and stellar content
- How Do Stars Form? Open Questions on the Stellar Initial Mass Function
- Weighing stars from birth to death: mass determination methods across the HRD
- A massive binary system with a single magnetic star
- State-of-the-art evolution models for single, binary and magnetic massive stars
- The young massive SMC cluster NGC 330 seen by MUSE. II. Multiplicity properties of the massive-star population
- Observational evidence of coalescence as a viable cause of magnetism in massive stars
- The Tarantula Massive Binary Monitoring. V. R 144: a wind-eclipsing binary with a total mass \ensuremath≳140 M_\ensuremath⊙
- Simulating the formation of \ensuremathη Carinae’s surrounding nebula through unstable triple evolution and stellar merger-induced eruption
- The Tarantula Massive Binary Monitoring. VI. Characterisation of hidden companions in 51 single-lined O-type binaries: A flat mass-ratio distribution and black-hole binary candidates
- Binary black hole mergers from merged stars in the Galactic field
- An X-ray-quiet black hole born with a negligible kick in a massive binary within the Large Magellanic Cloud
- The R136 star cluster dissected with Hubble Space Telescope/STIS. III. The most massive stars and their clumped winds
- Bipolar planetary nebulae from common-envelope evolution of binary stars
- Testing the evolution theory of massive binary systems
- Horizons: nuclear astrophysics in the 2020s and beyond
- TULIPS: A Tool for Understanding the Lives, Interiors, and Physics of Stars
- The young massive SMC cluster NGC 330 seen by MUSE. III. Stellar parameters and rotational velocities
- Bimodal Black Hole Mass Distribution and Chirp Masses of Binary Black Hole Mergers
- Gravitational wave emission from dynamical stellar interactions
- 3D simulations of strongly magnetized non-rotating supernovae: explosion dynamics and remnant properties
- The VLT-FLAMES Tarantula Survey. Observational evidence for two distinct populations of massive runaway stars in 30 Doradus
- From 3D hydrodynamic simulations of common-envelope interaction to gravitational-wave mergers
- The contribution of binary star formation via core fragmentation on protostellar multiplicity
- Nucleosynthesis of Binary-stripped Stars
- Bringing Stellar Evolution and Feedback Together: Summary of Proposals from the Lorentz Center Workshop
- X-Shooting ULLYSES: Massive stars at low metallicity. I. Project description
- Observations of high-order multiplicity in a high-mass stellar protocluster
- Contact tracing of binary stars: Pathways to stellar mergers
- Merger seismology: Distinguishing massive merger products from genuine single stars using asteroseismology
- Going from 3D Common-envelope Simulations to Fast 1D Simulations
- An interaction and merger in a massive multiple system create a magnetic field in a massive star
- From spherical stars to disk-like structures: 3D common-envelope evolution of massive binaries beyond inspiral
- Large-scale ordered magnetic fields generated in mergers of helium white dwarfs
- Binarity at LOw Metallicity (BLOeM): A spectroscopic VLT monitoring survey of massive stars in the SMC
- Merger seismology: Asteroseismic properties of massive merger products
- Primary and secondary source of energy in the superluminous supernova 2018ibb
- Evolution and final fate of massive post-common-envelope binaries
- Pre-supernova evolution and final fate of stellar mergers and accretors of binary mass transfer
- A magnetic massive star has experienced a stellar merger
- Towards a self-consistent model of the convective core boundary in upper main sequence stars. I. 2.5D and 3D simulations
- Going from 3D to 1D: A 1D approach to common-envelope evolution
- Faint calcium-rich transient from a double detonation of a 0.6 M_\ensuremath⊙ carbon-oxygen white dwarf star
- Convective-core overshooting and the final fate of massive stars
- Nitrogen abundances of the Be-type stars in 30 Doradus
- The evolution of binary-stripped stars: consequences for supernovae and black hole formation
- Contact Tracing of Massive Binary Stars
- Magnetic massive stars from stellar mergers
- The clumped winds of the most massive stars
- Scalable stellar evolution forecasting. Deep learning emulation versus hierarchical nearest-neighbor interpolation
- Self-consistent magnetohydrodynamic simulation of jet launching in a neutron star - white dwarf merger
- Clumping and X-rays in cooler B supergiant stars
- Finding the Fuse: Prospects for the Detection and Characterization of Hydrogen-rich Core-collapse Supernova Precursor Emission with the LSST
- Stripped Helium Star and Compact Object Binaries in Coeval Populations: Predictions Based on Detailed Binary Evolution Models
- Protostellar spin-up and fast rotator formation through binary star formation
- Orbital architectures of planet-hosting binaries – III. Testing mutual inclinations of stellar and planetary orbits in triple-star systems
- Simulated analogues I: apparent and physical evolution of young binary protostellar systems
- Simulated analogues II: a new methodology for non-parametric matching of models to observations
- Discovery of a septuple protostellar system--implications for the origin of extreme high-order multiplicity
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