D. Hutsemékers

collaborators

2 papers

astro-ph.HE2026

Radiation-pressure instability is an artifact of constant- $I^\pm$ closure. Implications for AGN disk tensions

M. H. Naddaf, M. Ghasemnezhad, H. Ghanbarnejad +2

The standard $I^\pm$ -disk formalism parametrizes turbulent angular momentum transport through a dimensionless coefficient $I^\pm$ , assumed to be spatially and thermodynamically invariant…

astro-ph.GA2025

H $I^^{2}$ line shape and radius-luminosity relation in 2.5D FRADO

M. H. Naddaf, M. L. Martinez-Aldama, D. Hutsemekers +2

Galaxies with active galactic nuclei (AGN) exhibit broad emission lines as a key spectral feature. The shape of emission-line profiles depends on the complex dynamics of discrete c…

Radiation-pressure instability is an artifact of constant-I^± closure. Implications for AGN disk tensions

HI^2 line shape and radius-luminosity relation in 2.5D FRADO

Radiation-pressure instability is an artifact of constant- $I^\pm$ closure. Implications for AGN disk tensions

H $I^^{2}$ line shape and radius-luminosity relation in 2.5D FRADO