arXiv:2508.21157v1 Announce Type: new Abstract: We investigate the impacts of the evolution of dust mass and grain size distribution within a Milky Way-like (MW-like) galaxy simulation on global atte...

arXiv:2508.21262v1 Announce Type: new Abstract: Microlensing induced by the stellar field within a strong lensing galaxy can introduce fluctuations in the waveforms of strongly-lensed gravitational w...

arXiv:2508.21282v1 Announce Type: new Abstract: Active galactic nuclei (AGN) jets are powerful drivers of galaxy evolution, depositing energy and momentum into the circumgalactic and intracluster med...

arXiv:2508.21229v1 Announce Type: new Abstract: We present spectroscopic identification of 43 quasars and 11 candidate obscured quasars in the epoch of reionization (EoR) at $5.71 \le z \le 7.02$, al...

arXiv:2508.21203v1 Announce Type: new Abstract: In this study, we present novel calculations of X-ray polarization from radio-quiet and unobscured active galactic nuclei (AGNs) using the Monte Carlo ...

arXiv:2508.21275v1 Announce Type: new Abstract: We present a fast and accurate formulation for computing the nonlinear matter power spectrum at one-loop order based on Unified Lagrangian Perturbation...

arXiv:2508.21194v1 Announce Type: new Abstract: Context. Central stars of planetary nebulae (CSPNe) are essential for understanding the final evolutionary stages of low- and intermediate-mass stars. ...

arXiv:2508.21116v1 Announce Type: new Abstract: We present a grid of rotating supergiant models from post-main sequence binary merger products, constructed by the MESA stellar evolution code. We focu...

arXiv:2508.21166v1 Announce Type: new Abstract: Photoevaporative models predict that the lower edge of the Neptune desert is sculpted by atmospheric mass loss. However, the stellar high energy fluxes...

arXiv:2508.21233v1 Announce Type: new Abstract: The initial mass and metallicity of stars both have a strong impact on their fate. Stellar axial rotation also has a strong impact on the structure and...