no code implementations • 18 Jan 2021 • Thomas A. Davison, Harald Kuntschner, Bernd Husemann, Mark A. Norris, Julianne J. Dalcanton, Alessandra De Rosa, Pierre-Alain Duc, Stefano Bianchi, Pedro R. Capelo, Cristian Vignali
The simultaneous advancement of high resolution integral field unit spectroscopy and robust full-spectral fitting codes now make it possible to examine spatially-resolved kinematic, chemical composition, and star-formation history from nearby galaxies.
Astrophysics of Galaxies