David R. Soderblom
Published 2014-09-08Version 1
Estimating ages for stars is difficult at best, but Galactic problems have their own requirements that go beyond those for other areas of astrophysics. As in other areas, asteroseismology is helping, and in this review I discuss some of the general problems encountered and some specific to large-scale studies of the Milky Way.
Comments: Proc. of the workshop "Asteroseismology of stellar populations in the Milky Way" (Sesto, 22-26 July 2013), Astrophysics and Space Science Proceedings, (eds. A. Miglio, L. Girardi, P. Eggenberger, J. Montalban)
The OGLE Collection of Variable Stars. Nearly 66,000 Mira stars in the Milky Way
Origin of the CEMP-no Group Morphology in the Milky Way
Table of Contents of: "Red Giants as Probes of the Structure and Evolution of the Milky Way"
![QR code for arXiv:1409.2266 [astro-ph.SR]](http://oss.arxitics.com/images/favicon.svg)