Gas flows in the central region of the Seyfert galaxy NGC 4593 with MUSE
Context. Understanding how gas flows into galactic centres, fuels the active galactic nucleus (AGN), and is in turn expelled back through feedback processes is of great importance to appreciate the role AGN play in the growth and evolution of galaxies. Aims. We use Multi Unit Spectroscopic Explorer-adaptive optics (MUSE-AO) optical spectra of the
Baki, P. et al.
Fecha de publicación:
10
2024