New ultraviolet spectra behind Andromeda reveal a corotating thick disk within 30 kpc and a radially stratified inner circumgalactic medium with no detected azimuthal dependence.
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7 Pith papers cite this work, alongside 159 external citations. Polarity classification is still indexing.
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astro-ph.GA 7representative citing papers
A single gas cloud at z=0.87641, seen in absorption against a quasar, sits at the edge of two galaxies' halos and matches the expected signature of cool gas flowing into them.
A new catalog of 389 isolated galaxies with clean 21-cm asymmetry measurements shows that low-mass asymmetric galaxies have elevated specific star formation, matching EAGLE predictions.
Cold filamentary accretion dominates gas supply in massive galaxies at z=2-4, and a double-sigmoid model describes how the cold fraction evolves with mass and redshift.
TNG50 simulation analysis finds early-forming halos show higher stellar mass, metallicity, lower CGM gas mass and sSFR at z=0, with mass-dependent CGM metallicity reversal and cold-gas kinematics differences.
IllustrisTNG simulations indicate galactic disk precession is common, driven by external tidal torques within 30 kpc, inducing warps and influencing evolution at all redshifts.
A unified empirical equation, fitted separately to three simulation suites, links galaxy star formation history shape to halo mass, baryon fraction, black hole mass, and feedback strength.
citing papers explorer
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A Partial Lyman Limit Absorber in the Halo of a Galaxy Pair: A Possible Signature of Gas Inflow
A single gas cloud at z=0.87641, seen in absorption against a quasar, sits at the edge of two galaxies' halos and matches the expected signature of cool gas flowing into them.
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Asymmetries in spatially unresolved 21-cm emission line profiles of isolated galaxies
A new catalog of 389 isolated galaxies with clean 21-cm asymmetry measurements shows that low-mass asymmetric galaxies have elevated specific star formation, matching EAGLE predictions.
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The dependence of Circumgalactic Medium properties on halo assembly histories in the IllustrisTNG simulations
TNG50 simulation analysis finds early-forming halos show higher stellar mass, metallicity, lower CGM gas mass and sSFR at z=0, with mass-dependent CGM metallicity reversal and cold-gas kinematics differences.
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A Universal Dance of Galactic Disks: Ubiquitous Precession and Its Implications
IllustrisTNG simulations indicate galactic disk precession is common, driven by external tidal torques within 30 kpc, inducing warps and influencing evolution at all redshifts.