Mapping the Youngest and Most Massive Stars in the Tarantula Nebula with MUSE-NFM
The evolution of the most massive stars is a puzzle with many missing pieces. Statistical analyses are key to providing anchors to calibrate theory, but performing these studies is an arduous job. The state-of-the-art integral field spectrograph Multi Unit Spectroscopic Explorer (MUSE) has stirred up stellar astrophysicists, who are excited about
Castro, N. et al.
Fecha de publicación:
3
2021