Results 61 to 70 of about 28,742 (262)
Massive runaways and walkaway stars
Anticipating the kinematic constraints from the Gaia mission, we perform an extensive numerical study of the evolution of massive binary systems to predict the peculiar velocities that stars obtain when their companion collapses and disrupts the system. Our aim is to (1) identify which predictions are robust against model uncertainties and assess their
Renzo, M. +8 more
openaire +2 more sources
Knowledge‐based atomistic workflows are presented for mechanical and thermodynamic properties. By coupling modular simulations with ontology‐aligned metadata and provenance, Fe case studies on elastic behavior, defects, thermal properties, and Hall–Petch strengthening reveal how FAIR, queryable, and reusable simulation data can be generated. Mechanical
Abril Azócar Guzmán +5 more
wiley +1 more source
Stellar wind yields of very massive stars
The most massive stars provide an essential source of recycled material for young clusters and galaxies. While very massive stars (VMS, M>100 $\rm {\rm M}_{\odot }$) are relatively rare compared to O stars, they lose disproportionately large ...
Hirschi, Raphael +4 more
core +1 more source
Molecular dynamics is used to investigate structure refinement during severe plastic deformation. The results show similitude with experimental data. Molecular dynamics simulations of severe plastic deformation of monocrystalline and polycrystalline samples by multiaxial compression of aluminum are carried out.
Roberto B. Figueiredo
wiley +1 more source
A novel phthalocyanine (PC)‐based metal–organic framework (MOFs) is synthesized using ditopic PC linkers obtained through regioselective statistical condensation. The resulting MOF exhibits significant improvements in electronic absorption, thereby enhancing the material's performance in light harvesting and energy conversion.
Lukas S. Langer +12 more
wiley +1 more source
Optimizing Image Fidelity with Arrays [PDF]
Through simulations, I have investigated the limitations imposed upon the image fidelity of interferometric observations by primary beam errors. Significant antenna surface and pointing errors lead to the greatest reduction in fidelity for most cases ...
Corder, Stuartt Allan
core +1 more source
VLTI view on evolved massive stars
Mass loss plays an important role in the evolution of massive stars. High angular resolution observations of the atmosphere, wind, and circumstellar environment of evolved massive stars allow us to improve our understanding of the mass-loss mechanism. We
Ohnaka, Keiichi
core +1 more source
The separation of Helium gas from natural gas is challenging but highly important. MIL‐116(Ga), a “non‐porous” metal–organic framework is used as a molecular sieve to separate He from CH4. Druse‐like MIL‐116(Ga) particles are integrated into polysulfone mixed matrix membranes.
Ayisha Komal +10 more
wiley +1 more source
Nuclear statistical equilibrium in massive stars: investigating the influence of electron fraction [PDF]
openUpon concluding the silicon burning phase, the core temperature and density in massive stars escalate to a level where nuclear statistical equilibrium is achieved.
MOGNOL, FEDERICO
core

