collaborators

12 papers

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

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.SR2026

High-fidelity stellar extinction with Gaia and APOGEE -- I. The method and a new extinction curve

Jie Yu, Luca Casagrande, John A. Taylor +9

The scarcity of high-fidelity extinction measurements remains a bottleneck in deriving accurate stellar properties from Gaia parallaxes. In this work, we aim to derive precision ex…

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

From Gaia to GaiaNIR: II. A new view of the Milky Way bar

Ó. Jiménez-Arranz, M. Schölch, S. Khanna +9

The Milky Way (MW) hosts a central bar whose pattern speed, orientation, and length remain uncertain, largely due to observational biases and selection effects, despite the transfo…

astro-ph.GA2026

The Effect of a Non-universal Extinction Curve on the Wesenheit Function and Cepheid Distances

D. M. Skowron, M. L. Fouesneau, R. Drimmel +1

The Wesenheit function is widely used to reduce the effects of interstellar reddening in distance measurements. Its construction, however, relies on the assumption of a universal e…