SMASHing the LMC: Mapping a Ring-like Stellar Overdensity in the LMC Disk
We explore the stellar structure of the Large Magellanic Cloud (LMC) disk using data from the Survey of the MAgellanic Stellar History and the Dark Energy Survey. We detect a ring-like stellar overdensity in the red clump star count map at a radius of ∼6° (∼5.2 kpc at the LMC distance) that is continuous over ∼270° in position angle and is only
Choi, Y. et al.
Fecha de publicación:
12
2018