arXiv:2508.15056v1 Announce Type: new Abstract: Context: Recent studies using Gaia data have reported tidal tail detections for tens to hundreds of open clusters. However, a comprehensive assessment ...
arXiv:2508.15063v1 Announce Type: new Abstract: We present the first results from the COSINE (Cometary Object Study Investigating their Nature and Evolution) project, based on a uniformly processed d...
arXiv:2508.15106v1 Announce Type: new Abstract: This study evaluates the performance of several machine learning models for predicting hazardous near-Earth objects (NEOs) through a binary classificat...
arXiv:2508.15173v1 Announce Type: new Abstract: Several models have been proposed to explain the formation of solar prominences, among which the evaporation--condensation model and the direct injecti...
arXiv:2508.15161v1 Announce Type: new Abstract: The young neutron star (NS) in the Cassiopeia A (Cas A) supernova remnant is a fascinating test for theories of NS cooling. Chandra observations have i...
arXiv:2508.15150v1 Announce Type: new Abstract: We present a pseudo-Newtonian stationary circumbinary slim disk model. We extend the slim disk formalism by including the binary tidal torque and solve...
arXiv:2508.15138v1 Announce Type: new Abstract: Galaxy cluster mergers drive powerful shock fronts that heat the Intra-Cluster Medium (ICM) and accelerate particles, redistributing the energy in a me...
arXiv:2508.15102v1 Announce Type: new Abstract: Here we present an open-source cloud model for substellar atmospheres, called Virga. The Virga-v0 series has already been widely adopted in the literat...
arXiv:2508.15134v1 Announce Type: new Abstract: We investigate whether an Early-Universe stochastic gravitational-wave background (SGWB) can account for the common spectrum process reported by NANOGr...
arXiv:2508.15107v1 Announce Type: new Abstract: Flares from stars can significantly impact the atmospheres of their orbiting planets, yet the role of hard X-ray (HXR; 3-20 keV) emission in driving es...