Solar twins in Gaia DR3 GSP-Spec II. Age distribution and its implications for the Sun's migration
arXiv:2603.11155 · doi:10.1051/0004-6361/202658914
Abstract
Solar twins are among the most powerful tracers of Galactic disk evolution owing to their unique property of sharing nearly solar metallicities ([Fe/H] ~ 0) while spanning a wide range of ages. To grasp solar twins as relics of Galaxy evolution, individual twins must be tagged with ages. A sufficiently large and well-characterized stellar sample then allows us to construct an age distribution that encodes the star formation history beyond our local region, modulated by the efficiency of radial migration of stars. Based on our catalog of 6,594 high-quality local (<~ 300 pc) solar twins from the Gaia Data Release 3 spectroscopic (GSP-Spec) catalog, we derived their age distribution after carefully deconvolving the selection function. We find two distinct features: a narrow peak around ~ 2 Gyr and a broad bump extending over ~ 4--6 Gyr. First, we argue that the former corresponds to a relatively recent burst of star formation that occurred in the disk, including at least a local region within a few kiloparsecs of the Sun, which is in good agreement with previous results deduced from independent works. On the other hand, the older bump, closely associated with the Sun's birth epoch, is intriguing since this finding challenges the predicted presence of a corotation barrier built by the Galactic bar, which is thought to prevent stars born inside R_GC ~ 6 kpc from reaching the solar neighborhood. We propose that the large number of local twins with ages between 4 and 6 Gyr provides compelling evidence that the Sun's long-distance (>= 3 kpc) migration is shared by many inner disk stars. This, in turn, suggests a possible link with the epoch of bar formation, which may have triggered enhanced star formation in the inner disk and induced efficient radial migration.
8 pages (main text 4 pages), 2+9 figures. Published in A&A
References in corpus (21)
- Riding the Spiral Waves: Implications of Stellar Migration for the Properties of Galactic Disks
- Dynamical modelling of the Galactic bulge and bar: the Milky Way's bar pattern speed, stellar, and dark matter mass distribution
- Gaia Data Release 3: Analysis of RVS spectra using the General Stellar Parametriser from spectroscopy
- A time-resolved picture of our Milky Way's early formation history
- From dawn till disk: Milky Way's turbulent youth revealed by the APOGEE+Gaia data
- Gaia DR2 reveals a star formation burst in the disc 2-3 Gyr ago
- The Pristine survey X: a large population of low-metallicity stars permeates the Galactic disk
- Resonances in Barred Galaxies
- Unveiling the time evolution of chemical abundances across the Milky Way disk with APOGEE
- Characterizing epochs of star formation across the Milky Way disc using age-metallicity distributions of GALAH stars
- On the origin of the Galactic thin and thick discs, their abundance gradients and the diagnostic potential of their abundance ratios
- Chronology of our Galaxy from Gaia Colour-Magnitude Diagram-fitting (ChronoGal). I. The formation and evolution of the thin disk from the Gaia Catalogue of Nearby Stars
- The Hercules stream as seen by APOGEE-2 South
- Observational Constraints of Radial Migration in the Galactic Disc Driven by the Slowing Bar
- Analytic solution of Chemical Evolution Models with Type Ia SNe
- Solar System Migration Points to a Renewed Concept: Galactic Habitable Orbits
- Exploring the impact of a rapidly decelerating bar on transforming bulge orbits into disc-like orbits
- Bar-driven dispersal of Galactic substructure
- Recent star formation episodes in the Galaxy: impact on its chemical properties and the evolution of its abundance gradient
- A Very Metal-poor RR Lyrae Star with a Disk Orbit Found in the Solar Neighborhood
- Joint inference of the Milky Way star formation history and IMF from Gaia all-sky data