GrW 231123 , the SIMBAD biblio

GrW 231123 , the SIMBAD biblio (28 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST09:13:14

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2025MNRAS.543.1833M 47           X         1 2 ~ Connecting the hierarchically merging binary black hole population to their host galaxies. MONCRIEFF J.W.N. and PANTHER F.H.
2025MNRAS.543.2796H 47           X         1 5 ~ The fate of rotating massive stars across cosmic times. HIRSCHI R., GOODMAN K., MEYNET G., et al.
2025ApJ...992L..26S 1567 T   A     X C       32 2 ~ Resolving Black Hole Family Issues among the Massive Ancestors of Very High-spin Gravitational-wave Events like
GW231123. 		STEGMANN J., OLEJAK A. and DE MINK S.E.
2025ApJ...993L..21A 280           X C       5 18 ~ GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-spin Black Hole Coalescences. ABAC A.G., ABOUELFETTOUH I., ACERNESE F., et al.
2025ApJ...993L..25A 3853 T   A     X C       81 2 ~
GW231123: A Binary Black Hole Merger with Total Mass 190-265 M⊙. 		ABAC A.G., ABOUELFETTOUH I., ACERNESE F., et al.
2025ApJ...993L..30L 2874 T   A     X C       60 1 ~ On the Formation of
GW231123 in Population III Star Clusters. 		LIU S., WANG L., TANIKAWA A., et al.
2025ApJ...993L..54G 1288 T   A     X C       26 4 ~ Spinning into the Gap: Direct-horizon Collapse as the Origin of
GW231123 from End-to-end General-relativistic Magnetohydrodynamic Simulations. 		GOTTLIEB O., METZGER B.D., ISSA D., et al.
2025ApJ...993..163C 280           X C       5 7 ~ McFACTS. II. Mass Ratio-Effective Spin Relationship of Black Hole Mergers in the Active Galactic Nucleus Channel. COOK H.E., McKERNAN B., FORD K.E.S., et al.
2025A&A...702A.208R 355     A S   X         7 1 ~ Black hole mass function shift in proto-stellar clusters driven by gas accretion. ROUPAS Z.
2025A&A...702A.233L 47           X         1 18 ~ Compact stellar systems hosting an intermediate-mass black hole: Magnetohydrodynamic study of inflow-outflow dynamics. LABAJ M., RESSLER S.M., ZAJACEK M., et al.
2025ApJ...994L..37K 308     A     X C       6 1 ~ Beyond Hierarchical Mergers: Accretion-driven Origins of Massive, Highly Spinning Black Holes in Dense Star Clusters. KIROGLU F., KREMER K. and RASIO F.A.
2025ApJ...994L..52T 47           X         1 2 ~ Where did Heavy Binaries Go? Gravitational-wave Populations Using Delaunay Triangulation with Optimized Complexity. TENORIO R., TOUBIANA A., BRUEL T., et al.
2025ApJ...994L..54P 2314 T   A     X C       48 3 ~ Assembling
GW231123 in Star Clusters through the Combination of Stellar Binary Evolution and Hierarchical Mergers. 		PAIELLA L., UGOLINI C., SPERA M., et al.
2025ApJ...994..261A 93           X         2 7 ~ Do Both Black Holes Spin in Merging Binaries? Evidence from GWTC-4 and Astrophysical Implications. ADAMCEWICZ C., GUTTMAN N., LASKY P.D., et al.
2025ApJ...995L...6C 914 T   A     X C       18 1 ~ Machine Learning Confirms
GW231123 is a “Lite” Intermediate Mass Black Hole Merger. 		CHATTERJEE C., McGOWAN K., DESHMUKH S., et al.
2025ApJ...995L..18A 93           X         2 10 ~ GWTC-4.0: An Introduction to Version 4.0 of the Gravitational-Wave Transient Catalog. ABAC A.G., ABOUELFETTOUH I., ACERNESE F., et al.
2025ApJ...995L..76P 1241 T   A     X C       25 1 ~ Very Massive, Rapidly Spinning Binary Black Hole Progenitors through Chemically Homogeneous Evolution-The Case of
GW231123. 		POPA S.A. and DE MINK S.E.
2026ApJ...996L...4M 1080     A     X C       21 2 ~ What is the Most Massive Gravitational-wave Source? MANDEL I.
2026ApJ...996...57S 380     A     X         8 2 ~ Collapse of Rotating Very Massive Stellar Cores Leading to a Black Hole and a Massive Disk as a Source of Gravitational Waves. SHIBATA M. and FUJIBAYASHI S.
2026ApJ...996L..44B 1580 T   A     X C       30 2 ~ Accretion is All You Need: Black Hole Spin Alignment in Merger
GW231123 Indicates Accretion Pathway. 		BARTOS I. and HAIMAN Z.
2026ApJ...996..142H 50           X         1 4 ~ Accretion Regimes of Neutrino-cooled Flows onto Black Holes. HERNANDEZ-MORALES J. and SIEGEL D.M.
2026ApJ...996..144G 50           X         1 2 ~ Trends in the Population of Binary Black Holes Following the Fourth Gravitational-wave Transient Catalog: A Data-driven Analysis. GUTTMAN N., PAYNE E., LASKY P.D., et al.
2026ApJ...998..138M 530     A     X C       10 9 ~ Shadows of the Colossus: Hierarchical Black Hole Mergers in a 10-million-body Globular Cluster Simulation. MAI A., KREMER K. and KIROGLU F.
2026ApJ...999..127L 3130 T   A     X C       61 2 ~
GW231123: Likely a Product of Successive Mergers from ∼10 Stellar-mass Black Holes. 		LI Y.-J., TANG S.-P., XUE L.-Q., et al.
2026ApJ...999L..30V 100           X         2 3 ~ The Maximum Mass Ratio of Hierarchical Binary Black Hole Mergers May Cause the q-χeff Correlation. VIJAYKUMAR A., FARAH A.M. and FISHBACH M.
2026ApJ...999..236P 2580 T   A     X C       50 1 ~ Is
GW231123 a Hierarchical Merger? 		PASSENGER L., BANAGIRI S., THRANE E., et al.
2026ApJ..1000...77L 50           X         1 6 ~ Accretion-modified Stars in Accretion Disks of Active Galactic Nuclei: Contribution to Active Galactic Nuclei Disk Viscosity. LIU J.-R., WANG J.-M. and FENG H.
2026A&A...707A..38T 480     A S   X C       8 9 ~ Optically thick winds of very massive stars suppress intermediate-mass black hole formation. TORNIAMENTI S., MAPELLI M., BOCO L., et al.

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