Image Details
Caption: Figure 5.
Map of the MCs using RG stars selected with Gaia DR3. Left: stars in the Magellanic periphery extend to at least ∼20° around the LMC and organize into many diffuse substructures. The origin of these features is not well understood. Right: distribution of 109,188 MC RG stars observed by BOSS.
© 2026. The Author(s). Published by the American Astronomical Society.