output
20082026
most citedConstraints on galaxy formation models from the galaxy stellar mass function and its evolution

39 citations

15 papers

gr-qc2026

Hawking atmosphere of anti-de Sitter black holes

A. F. Cardona, C. Molina

This work investigates the semiclassical evolution of the Hawking atmosphere surrounding evaporating, spherically symmetric anti-de Sitter (adS) black holes. We model the evaporati…

astro-ph.HE2026

Is plasmoid-mediated reconnection really important in accretion flows to drive flares in AGNs?

Giovani H. Vicentin, Elisabete M. de Gouveia Dal Pino, George N. Wong +4

Based on very high-resolution resistive 2D and 3D magnetohydrodynamical (MHD) simulations of current sheets, our findings suggest that the answer to this question is likely no. In…

physics.plasm-ph2025★ 3 cited

Do plasmoids induce fast magnetic reconnection in well-resolved current sheets in 2D MHD simulations?

G. H. Vicentin, G. Kowal, E. M. de Gouveia Dal Pino +1

We investigate the development of tearing-mode instability using the highest-resolution two-dimensional magnetohydrodynamic simulations of reconnecting current sheets performed on…

astro-ph.HE2025

Correlating Particle Acceleration Rates with Plasma Conditions in Colliding Wind Binaries

Gislaine B Cordeiro, Diego Falceta-Gonçalves, Grzegorz Kowal +1

Recent observations have revealed star-forming regions as possible origin sites of very-high-energy (TeV) cosmic rays, not associated with supernova remnants. Colliding-wind binari…

astro-ph.HE2025★ 3 cited

Prospects for dark matter observations in dwarf spheroidal galaxies with the Cherenkov Telescope Array Observatory

K. Abe, S. Abe, J. Abhir +491

The dwarf spheroidal galaxies (dSphs) orbiting the Milky Way are widely regarded as systems supported by velocity dispersion against self-gravity, and as prime targets for the sear…

astro-ph.SR2025★ 2 cited

CGCS 6306, another X-ray-emitting asymptotic giant branch star confirmed to be a symbiotic binary

Jaroslav Merc, Martín A. Guerrero, Jesús A. Toalá +1

A number of asymptotic giant branch (AGB) stars are known to exhibit UV excess and/or X-ray emission. These have been considered signposts of a hot white dwarf (WD) companion in a…