Speaker
Smrithi Gireesh
(University of Sydney)
Description
I present a novel approach to classify stellar streams and shells using the clustering algorithm AstroLink. This density-driven approach is applied to tidally disrupted stellar shells and streams formed in mock MW static haloes. AstroLink can identify the structures formed from the N-body simulations and provide clues to identifying streams and shells based on the ordered density distribution. This work is currently submitted to PASA for publication.
Author
Smrithi Gireesh
(University of Sydney)
