Results 41 to 50 of about 916 (166)
We propose a formation pathway linking black holes (BHs) observed in gravitational-wave (GW) mergers, wide BH–stellar systems uncovered by Gaia, and accreting low-mass X-ray binaries (LMXBs).
Smadar Naoz +3 more
doaj +1 more source
Extreme emission line galaxies (EELGs), where nebular emissions contribute 30%–40% of the flux in certain photometric bands, are ubiquitous in the early Universe ( z > 6).
Anshu Gupta +9 more
doaj +1 more source
On the Formation of GW231123 in Population III Star Clusters
GW231123 is a binary black hole (BBH) merger whose primary component lies within or above the pair-instability mass gap, while the secondary component falls within this gap.
Shuai Liu +4 more
doaj +1 more source
Overmassive Supermassive Black Holes in SDSS Close Galaxy Pairs
Supermassive black holes (SMBHs) and their host galaxies coevolve through channels such as hierarchical merging and active galactic nuclei (AGN) feedback, establishing tight scaling relations between SMBH masses and the properties of the host galaxies ...
Maggie C. Huber +2 more
doaj +1 more source
The major merger–active galactic nucleus connection up to cosmic noon
Galaxy major mergers are a potential mechanism for triggering active galactic nuclei (AGN) activity, but their role remains debated, particularly beyond the local Universe.
La Marca A. +5 more
doaj +1 more source
The Role of Cluster Environments in Quiescent Galaxy Stellar Halo Assembly
External interactions drive galaxy stellar mass growth and morphological evolution. As stellar halos—assembled largely via hierarchical accretion—preserve signatures of these processes, their growth probes how environment regulates galaxy evolution.
Devin J. Williams +8 more
doaj +1 more source
Bulgeless Evolution And the Rise of Discs (BEARD)
We study the formation and evolution of bulgeless galaxies within the Milky Way-Andromeda analogue sample of the TNG50 simulation. Through kinematic decomposition with MORDOR, we identified bulgeless galaxies with a bulge-to-disc mass ratio of B/D ≤ 0.08,
Rosas-Guevara Yetli +22 more
doaj +1 more source
We present a resolved study of 877 progenitors of Milky Way Analogs (MWAs) at 0.3
Vivian Yun Yan Tan +19 more
doaj +1 more source
The Mass Density of Merging Binary Black Holes over Cosmic Time
The connection between the binary black hole (BBH) mergers observed by LIGO-Virgo-KAGRA and their stellar progenitors remains uncertain. Specifically, the fraction ϵ of stellar mass that ends up in BBH mergers and the delay time τ between star formation ...
Aryanna Schiebelbein-Zwack +1 more
doaj +1 more source
Theory, Simulations, and Observations of Stellar Mergers
Stellar mergers are responsible for a great variety of astrophysical phenomena. They form blue straggler stars, give rise to spectacular transients, and produce some of the most massive stars in the Universe. Here, we focus on mergers from binary evolution and stellar collisions but do not cover mergers involving compact objects ...
openaire +2 more sources

