SMUGGLE-Ring: Evolutionary link between nuclear star cluster and nuclear disk

Kavli Affiliate: Mark Vogelsberger | Summary:We present a high-resolution hydrodynamical simulation of the formation and evolution of nuclear structures in a Milky Way-mass galaxy using the SMUGGLE multiphase ISM and stellar feedback model. The system naturally develops a bar of length $approx5$ kpc in isolation, driving sustained gas inflows toward the center that lead to […]


Continue.. SMUGGLE-Ring: Evolutionary link between nuclear star cluster and nuclear disk

SMUGGLE-Ring: Evolutionary link between nuclear star cluster and nuclear disk

Kavli Affiliate: Mark Vogelsberger | Summary:We present a high-resolution hydrodynamical simulation of the formation and evolution of nuclear structures in a Milky Way-mass galaxy using the SMUGGLE model. The system naturally develops a bar in isolation of $approx5$ kpc in length, driving sustained gas inflows toward the center that lead to the formation of a […]


Continue.. SMUGGLE-Ring: Evolutionary link between nuclear star cluster and nuclear disk

The Role of Stellar Spin in Repeating Partial Tidal Disruption Events

Kavli Affiliate: Dheeraj Pasham | Summary:The repeated tidal stripping of a star by a supermassive black hole, known as a repeating partial tidal disruption event (rpTDE), can give rise to a transient that rebrightens months to years after the first outburst. Among the rpTDE candidates so far observed, some exhibit dimmer peak luminosities during each […]


Continue.. The Role of Stellar Spin in Repeating Partial Tidal Disruption Events

The Role of Stellar Spin in Repeating Partial Tidal Disruption Events

Kavli Affiliate: Dheeraj Pasham | Summary:The repeated tidal stripping of a star by a supermassive black hole, known as a repeating partial tidal disruption event (rpTDE), can give rise to a transient that rebrightens months to years after the first outburst. Among the rpTDE candidates so far observed, some exhibit dimmer peak luminosities during each […]


Continue.. The Role of Stellar Spin in Repeating Partial Tidal Disruption Events

Mergers Matter: Gravothermal Collapse in Dwarf Halos with Self-Interacting Dark Matter

Kavli Affiliate: Lina Necib | Summary:Self-Interacting Dark Matter (SIDM) models with large cross sections at relative velocities below $sim100,rm km , s^-1$ can be tested with dwarf galaxy observations. We analyze six dark-matter-only zoom-in $sim10^10,rm M_odot$ halos with diverse assembly histories, adopting a cross section over mass of $σ/m = 70,cm^2 , g^-1$. We find […]


Continue.. Mergers Matter: Gravothermal Collapse in Dwarf Halos with Self-Interacting Dark Matter

The Pan-Pacific Planet Search — IX. A menagerie of companions orbiting evolved stars

Kavli Affiliate: Avi Shporer | Summary:We present resolutions as to the nature of six speculative candidate companions proposed in the final data release of the Pan-Pacific Planet Search, a 6-year radial-velocity survey of 164 southern evolved stars using the now-decommissioned UCLES spectrograph on the 3.9m Anglo-Australian Telescope. New radial-velocity observations, TESS asteroseismology, and Hipparcos-Gaia astrometry […]


Continue.. The Pan-Pacific Planet Search — IX. A menagerie of companions orbiting evolved stars

A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones

Kavli Affiliate: Michael McDonald | Summary:Galaxy cluster strong gravitational lensing plays a central role in precision cosmology, yet robust theoretical predictions have lagged behind an abundance of high-quality strong lensing observations. This shortfall reflects both a mismatch between the geometry of the strong-lensing problem and standard cubic simulation boxes, and the fundamental tension between simulation […]


Continue.. A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones

A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones

Kavli Affiliate: Michael McDonald | Summary:Galaxy cluster strong gravitational lensing plays a central role in precision cosmology, yet robust theoretical predictions have lagged behind an abundance of high-quality strong lensing observations. This shortfall reflects both a mismatch between the geometry of the strong-lensing problem and standard cubic simulation boxes, and the fundamental tension between simulation […]


Continue.. A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones

The Lumina Project: The Demographics of Active Galactic Nuclei from Quasars to Little Red Dots at $zgeq 3$

Kavli Affiliate: Mark Vogelsberger | Summary:High-redshift active galactic nuclei (AGN) serve as powerful probes of early black-hole growth, galaxy formation, and the evolving intergalactic medium (IGM). In this work, we use Lumina, a cosmological radiation-hydrodynamic simulation spanning the epochs of hydrogen and helium reionization, which combines a large $(500,rm cMpc)^3$ volume with $2times 6000^3$ resolution […]


Continue.. The Lumina Project: The Demographics of Active Galactic Nuclei from Quasars to Little Red Dots at $zgeq 3$