An enquiry on the origins of N-rich stars in the inner Galaxy based on APOGEE chemical compositions
Recent evidence based on APOGEE data for stars within a few kpc of the Galactic Centre suggests that dissolved globular clusters (GCs) contribute significantly to the stellar mass budget of the inner halo. In this paper, we enquire into the origins of tracers of GC dissolution, N-rich stars, that are located in the inner 4 kpc of the Milky Way
Kisku, Shobhit et al.
Fecha de publicación:
6
2021