Abstract High-resolution observations of ionized and molecular gas in the nuclear regions galaxies are indispensable for delineating interplay star formation, gaseous inflows, stellar radiation, feedback processes. Combining our new Atacama Large Millimeter/submillimeter Array band 3 mapping archival Very Telescope/MUSE data, we present a spatially resolved analysis central 5.4 kpc region NGC 1...

Changing-look active galactic nuclei (CLAGNs) show a complex nature in their X-ray spectral shape and line-of-sight column-density variation. The physical mechanisms responsible for these variations are unclear. Here, we study the properties of CLAGN, NGC 1365 using combined XMM-Newton NuSTAR observations to understand CL behavior. model-fitted mass-accretion rate varied between 0.003 ± 0.001 0...

A primary new capability of JWST is the ability to penetrate dust in star forming galaxies identify and study properties young clusters that remain embedded gas. In this paper we combine infrared images taken with our optical HST star-bursting barred (Seyfert2) spiral galaxy NGC 1365. We find has richest population massive any known within 30 Mpc, $\sim$ are more than 10$^6$ Msolar younger 10 M...