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20242026
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astro-ph.GA2026

The Age-Thickness Relation as a Tracer of the Merger History of Disk Galaxies

Lekshmi Thulasidharan, Elena D'Onghia, Robert Benjamin +2

In the hierarchical framework of galaxy formation, disk galaxies are shaped by a sequence of mergers and interactions, yet reconstructing this history from observations remains cha…

astro-ph.GA2026

Unveiling the Milky Way with a Gaia DR3 census of OB-type stars within 2 kpc. I. Tracing local Galactic structure, massive star-forming regions and core-collapse supernova progenitors

Alexis L. Quintana, Kiril Maltsev, Eloisa Poggio +10

O- and B-type stars are young and hot, thereby serving as vital tracers of the star formation and spiral arm structure of the Milky Way. At the dusk of the \textit{Gaia} DR3 era, a…

astro-ph.GA2026

Rogue Ones: Orbital census of Galactic Cepheids and their Anomalies

Shourya Khanna, Ronald Drimmel, Eloisa Poggio +2

Classical Cepheids (DCEPs) are excellent standard candles expected to trace the spatial and kinematic distribution of the Galaxy's young and dynamically cold stellar disc. Using th…

astro-ph.GA2026

The flare and spiral structure of the Milky Way's disc as traced by young giant stars

E. Poggio, R. Drimmel, S. Khanna +2

We explore the three-dimensional structure of a sample of 16000 young giant stars in the Galactic disc out to 8 kpc in heliocentric distance. This population traces a…

astro-ph.GA2026

Classical Cepheids in the Galactic thin disk I. Abundance gradients via non-local thermodynamic equilibrium spectral analysis

Antonino Nunnari, Valentina D'Orazi, Giuliana Fiorentino +23

Classical Cepheids (CCs) have long been considered excellent tracers of the chemical evolution of the Milky Way's young disk. We present a homogeneous, NLTE spectroscopic analysis…

astro-ph.GA2025

GaiaUnlimited: The old stellar disc of the Milky Way as traced by the Red Clump

Shourya Khanna, Jie Yu, Ronald Drimmel +9

We present an exploration of the Milky Way's structural parameters using an all-sky sample of RC giants to map the stellar density from the Galactic disc beyond 3 kpc. These evolve…