Results 41 to 50 of about 3,286 (161)
We present results from the Cosmic Evolution Early Release Survey on the stellar population parameters for 28 galaxies with redshifts 4 < z < 9 using imaging data from the James Webb Space Telescope (JWST) Mid-Infrared Instrument (MIRI) combined with ...
Casey Papovich +48 more
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The energetics, evolution, and stellar depletion of $\mathsf{^6}$Li in the early Galaxy [PDF]
12 pages, 4 figures, final version after language editing for Astronomy and Astrophysics; references ...
openaire +3 more sources
The cosmic evolution of the stellar mass–velocity dispersion relation of early-type galaxies
ABSTRACTWe study the evolution of the observed correlation between central stellar velocity dispersion σe and stellar mass M* of massive ($M_*\gtrsim 3\times 10^{10}\, \mathrm{M_\odot}$) early-type galaxies (ETGs) out to redshift z ≈ 2.5, taking advantage of a Bayesian hierarchical inference formalism.
Carlo Cannarozzo +2 more
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The stellar Rossby number, a dimensionless parameter quantifying the influence of Coriolis forces on convective motions, plays a pivotal role in understanding magnetic stellar evolution.
Alfio M. Bonanno +5 more
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Within the lambda cold dark matter (ΛCDM) cosmological framework, the interplay between galaxy morphology, stellar mass, and environment remains uncertain at z > 1.
Fang Guanwen +4 more
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The formation and early dynamical evolution of bound stellar systems
We present the results of numerical N-body calculations which simulate the dynamical evolution of young clusters as they emerge from molecular clouds. We follow the evolution of initially virialized stellar systems of 50 and, in some cases, 100 stars from the point in time immediately after the stars have formed in a cloud until a time long after all ...
C. J. Lada, M. Margulis, D. Dearborn
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Coevolution of Nuclear Star Clusters and Massive Black Holes: Extreme-mass-ratio Inspirals
We explore extreme-mass-ratio inspirals (EMRIs) in the coevolution of massive black holes (MBHs) and nuclear star clusters (NSCs), which host diverse stellar populations across a wide range of masses. The dynamics are simulated self-consistently with GNC
Fupeng Zhang, Pau Amaro Seoane
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Revisiting the dynamics of planets in binaries: evolutionary timescales and the effect of early stellar evolution [PDF]
20 pages, 7 figures, Submitted to ...
Bayron Portilla-Revelo, Jorge I Zuluaga
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Recycled Gas Dominates the Metal-rich Fuel of Supermassive Black Holes
Understanding the origin and chemical properties of gas accreted by supermassive black holes (SMBHs) is essential for linking black hole growth to galaxy evolution.
Dongyun Kwak +7 more
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The evolution of high-z proto-star clusters into local globular clusters
The James Webb Space Telescope (JWST) detected numerous massive and relatively compact stellar clumps around proto-galaxies at high redshift (z > 0.5).
Della Croce A. +6 more
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