collaborators

8 papers

astro-ph.GA2025

Rediscovering the Milky Way with an orbit superposition approach and APOGEE data V. The disc growth and history of star formation

Bridget Ratcliffe, Sergey Khoperskov, Nathan Lee +8

The Milky Way's (MW's) star formation history (SFH) offers insight into the chronology of its assembly and the mechanisms driving its structural development. In this study, we pres…

astro-ph.GA2025

Bar-spiral interaction produces radial migration and star formation bursts

Léa Marques, Ivan Minchev, Bridget Ratcliffe +8

Central bars and spirals are known to strongly impact the evolution of their host galaxies, both in terms of dynamics and star formation. Their typically different pattern speeds c…

astro-ph.GA2024

Rediscovering the Milky Way with orbit superposition approach and APOGEE data III. Panoramic view of the bulge

Sergey Khoperskov, Paola Di Matteo, Matthias Steinmetz +9

The innermost parts of the Milky Way (MW) are very difficult to observe due to the high extinction along the line of sight, especially close to the disc mid-plane. However, this re…

astro-ph.GA2024

Rediscovering the Milky Way with orbit superposition approach and APOGEE data II. Chrono-chemo-kinematics of the disc

Sergey Khoperskov, Matthias Steinmetz, Misha Haywood +9

The stellar disc is the dominant luminous component of the Milky Way (MW). Although our understanding of its structure is rapidly expanding due to advances in large-scale stellar s…

astro-ph.GA2024

Rediscovering the Milky Way with orbit superposition approach and APOGEE data I. Method validation

Sergey Khoperskov, Glenn van de Ven, Matthias Steinmetz +9

We introduce a novel orbit superposition method designed to reconstruct the stellar density structure, kinematics, and chemical abundance distribution of the entire Milky Way by le…

astro-ph.GA2024

The chemical evolution of the Milky Way thin disk using solar twins

Anastasiia Plotnikova, Lorenzo Spina, Bridget Ratcliffe +2

In this study we address whether the age--metallicity relation (AMR) deviates from the expected trend of metallicity increasing smoothly with age. We also show the presence (or abs…