Milky Way's Thick and Thin disk: Is there distinct thick disk?
D. Kawata (MSSL, UCL), C. Chiappini (AIP)

TL;DR
This paper discusses whether the Milky Way has a distinct thick disk, highlighting different definitions, open questions about origins, and the importance of diverse modeling approaches in understanding galactic structure.
Contribution
It synthesizes expert discussions on the nature of the Milky Way's disks, emphasizing the need for multiple modeling approaches to address unresolved questions.
Findings
Existence of at least two different types of disks in the Milky Way
Open questions on defining and understanding the origins of these disks
Importance of diverse modeling approaches in galactic studies
Abstract
This article is based on our discussion session on Milky Way models at the 592 WE-Heraeus Seminar, Reconstructing the Milky Way's History: Spectroscopic Surveys, Asteroseismology and Chemodynamical models. The discussion focused on the following question: "Are there distinct thick and thin disks?". The answer to this question depends on the definition one adopts for thin and thick disks. The participants of this discussion converged to the idea that there are at least two different types of disks in the Milky Way. However, there are still important open questions on how to best define these two types of disks (chemically, kinematically, geometrically or by age?). The question of what is the origin of the distinct disks remains open. The future Galactic surveys which are highlighted in this conference should help us answering these questions. The almost one-hour debate involving…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
