A Radial Age Gradient in the Geometrically Thick Disk of the Milky Way
- Publisher: American Astronomical Society; IOP Publishing
QB | QC | QD | Astrophysics - Astrophysics of Galaxies
arxiv: Astrophysics::Galaxy Astrophysics | Astrophysics::Cosmology and Extragalactic Astrophysics | Astrophysics::Earth and Planetary Astrophysics | Astrophysics::Solar and Stellar Astrophysics
In the Milky Way, the thick disk can be defined using individual stellar abundances, kinematics, or age; or geometrically, as stars high above the mid-plane. In nearby galaxies, where only a geometric definition can be used, thick disks appear to have large radial scale...