The Milky Way's Stellar Disk

TL;DR

The paper reviews how stellar surveys, especially Gaia, enhance understanding of the Milky Way's stellar disk, emphasizing modeling techniques, the importance of selection functions, and the use of mono-abundance populations to study galaxy evolution and dark matter.

Contribution

It advocates for the use of mono-abundance populations in modeling the Galactic disk and discusses the necessary analysis tools to constrain galaxy evolution and dark matter distribution.

Findings

MAPs help disentangle disk structure and evolution

Survey selection functions are crucial for accurate modeling

Future Gaia data will clarify the Milky Way's formation history

Abstract

A suite of vast stellar surveys mapping the Milky Way, culminating in the Gaia mission, is revolutionizing the empirical information about the distribution and properties of stars in the Galactic stellar disk. We review and lay out what analysis and modeling machinery needs to be in place to test mechanisms of disk galaxy evolution and to stringently constrain the Galactic gravitational potential, using such Galactic star-by-star measurements. We stress the crucial role of stellar survey selection functions in any such modeling; and we advocate the utility of viewing the Galactic stellar disk as made up from `mono-abundance populations' (MAPs), both for dynamical modeling and for constraining the Milky Way's evolutionary processes. We review recent work on the spatial and kinematical distribution of MAPs, and lay out how further study of MAPs in the Gaia era should lead to a decisively clearer picture of the Milky Way's dark matter distribution and formation history.