Age Gradients Throughout the Galaxy with O-Miras
J. Grady, V. Belokurov, N.W. Evans (IoA, Cambridge)

TL;DR
This study uses a large sample of oxygen-rich Miras to map age gradients across the Galaxy, revealing how their periods correlate with galactic structure and identifying distant and extragalactic populations.
Contribution
It provides the largest catalog of O-Miras, demonstrating their effectiveness as age indicators for Galactic components and uncovering new distant and extragalactic Mira populations.
Findings
Outer disk O-Miras are younger than inner disk ones.
Transition from disk to halo occurs at ~15 kpc with period drop.
Presence of young O-Miras at high Galactic latitudes.
Abstract
We assemble the largest sample of oxygen rich Miras to date and highlight their importance for age-dating the components of the Galaxy. Using data from the Catalina Rapid Transient Survey and the All Sky Automated Survey for Supernovae, we extract a clean sample of O-Miras, stretching from the Galactic Bulge to the distant halo. Given that the period of O-Miras correlates with age, this offers a new way of determining age gradients throughout the Galaxy. We use our sample to show (i) disk O-Miras have periods increasing on moving outwards from ~ 3 to 15 kpc, so the outer disk O-Miras are younger than the inner disk, (ii) the transition from younger disk to halo O-Miras occurs at r ~ 15 kpc and is marked by a plummeting in period, (iii) there exists a population of young O-Miras likely kicked from the disk to heights of order of |Z| ~ 10 kpc, (iv) great circle counts of old…
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