Discovery and characterization of the highest-redshift barred spiral galaxy candidate at z=5.102, with bar length ~4.5 kpc, stellar mass 10^10.45 solar masses, SFR 144 solar masses per year, and evidence for AGN and interaction.
title Bi-symmetric instabilities of the Kuz 'min/ Toomre disc
5 Pith papers cite this work, alongside 193 external citations. Polarity classification is still indexing.
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GalPort computes multi-timescale action-angle variables and orbital classifications for evolving barred galaxy simulations, with specialised bar phase-space analysis tools.
Generalized linear matrix method computes normal modes in stellar disks with sharp L=0 edges via boundary integrals, validated to ~0.003 accuracy on Kuzmin-Toomre models against an independent nonlinear method.
Improved VMC proper motions show SMC expansion along SE-NW axes consistent with LMC tides, radial inward motions with no rotation, and northward motion in older RGB stars from a prior interaction.
A review summarizing detection methods, population statistics, and coevolution of supermassive black holes with host galaxies from early universe observations and simulations.
citing papers explorer
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A massive barred spiral galaxy at z = 5.102 discovered by JWST
Discovery and characterization of the highest-redshift barred spiral galaxy candidate at z=5.102, with bar length ~4.5 kpc, stellar mass 10^10.45 solar masses, SFR 144 solar masses per year, and evidence for AGN and interaction.
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GalPort: Investigation of the bar in action-angle space
GalPort computes multi-timescale action-angle variables and orbital classifications for evolving barred galaxy simulations, with specialised bar phase-space analysis tools.
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A generalized linear matrix method for normal modes in collisionless stellar disks
Generalized linear matrix method computes normal modes in stellar disks with sharp L=0 edges via boundary integrals, validated to ~0.003 accuracy on Kuzmin-Toomre models against an independent nonlinear method.
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The VMC survey -- LV. The coherent expansion of the SMC
Improved VMC proper motions show SMC expansion along SE-NW axes consistent with LMC tides, radial inward motions with no rotation, and northward motion in older RGB stars from a prior interaction.
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Massive black holes and their galaxies
A review summarizing detection methods, population statistics, and coevolution of supermassive black holes with host galaxies from early universe observations and simulations.