text: 27,185,1361560280828846081,1114972720826068992,Danny Horta Darrington 🇺🇦,"What's that, stars in the inner Milky Way that come from GCs and from an accreted origin? Check out some awesome results in a paper led by my PhD sibling Shobhit Kisku where we study the nature of chemically tagged dissolved GC stars in the inner Galaxy <LINK> @kaosteorin Thanks @kaosteorin !! I will make sure to pass the message on to Shobhit. Let us know if you wanna chat about it!",https://arxiv.org/abs/2102.06720,"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. From an analysis of the chemical compositions of these stars we establish that about 30% of the N-rich stars previously identified in the inner Galaxy may have an accreted origin. This result is confirmed by an analysis of the kinematic properties of our sample. The specific frequency of N-rich stars is quite large in the accreted population, exceeding that of its in situ counterparts by near an order of magnitude, in disagreement with predictions from numerical simulations. We hope that our numbers provide a useful test to models of GC formation and destruction. ","An enquiry on the origins of N-rich stars in the inner Galaxy basedon