Dust in the central parsecs of unobscured AGN: more challenges to the torus
A parsec-scale dusty torus is thought to be the cause of active galactic nuclei (AGN) dichotomy in the 1/2 types, narrow/broad emission lines. In a previous work, on the basis of parsec-scale resolution infrared/optical dust maps, it was found that dust filaments, few parsecs wide and several hundred parsecs long, were ubiquitous features crossing
Prieto, M. Almudena et al.
Fecha de publicación:
9
2021