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- A Century of Novae in the Large Magellanic Cloud
- Dynamical friction in stratified stellar envelopes
- The black hole occupation fraction as a fossil record of seeding, dynamics, and galaxy assembly
- The chemo-dynamical complexity of ω Centauri: different kinematics for different populations
- Evidence for phenylium reactivity under interstellar-relevant conditions
- Deep learning from the crowd Fundamentals of morphological galaxy classification
- Elusive helium stars in the gap between subdwarfs and Wolf-Rayet stars III. Formation of the Galactic population of stripped helium stars
- Fractional Bose-Einstein Condensate Dark Matter Cores: Numerical GPP Solutions and SPARC Rotation Curves
- Calibration of CNEOS Fireball Velocities and the Robustness of Nominally Hyperbolic Events
- ADF22-WEB: Massive galaxy formation shaped by cosmic web filaments in the z = 3.1 proto-cluster core
- Chandra X-ray imaging and IC/CMB model for the inner jet of PKS 0637-752
- DustRover: A Python Package for Modelling Dust Extinction Curves (Phase I)
- PERRY: A Human-in-the-Loop GUI for Precision Alignment of MUSE Data
- Rapid Growth of Intermediate-Mass Black Holes through Disk-induced Stellar Disruptions
- Magnetic Fields in Massive Star-forming Regions (MagMaR). IX. Radiative Torque Alignment and Disruption in NGC6334I
- Tidal origin of dark-matter free dwarf galaxies in the NGC 1052 group
- Connecting the little dots in polarized light
- Shaving the Outskirts of Planetary Systems Probed by Roman via Stellar Flybys
- FAST Observations of Filamentary and Compact H I Structure in a Magellanic Stream IV Field
- Self-supervised reconstruction of transients in data from space-borne gravitational-wave detectors
- A Uniform Census of Variable Stars in M101 Based on HST/ACS Photometry
- Multi-epoch Detection of an Ultra-fast Inflow in ESP 39607: Evidence for an Accretion Cascade
- Serendipitous discovery of an almost-dark galaxy in the Virgo Cluster
- Hydrodynamical mass-loss rates for Very Massive Stars II. New theoretical mass-loss predictions at solar metallicity (Z = 0.02)
- Halo-driven Origin and Evolution of Overmassive Black Holes and Little Red Dots