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Chronology of our Galaxy from Gaia colour-magnitude diagram fitting (ChronoGal)

The Milky Way’s inner region is dominated by a stellar bar and a boxy-peanut-shaped bulge. However, which stellar populations inhabit the inner Galaxy or how star formation proceeded there is still unknown. The difficulty in studying these stars stems from their location in dense regions that are st...

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Autori principali: Ruiz-Lara Tomás, Mirabal David, Gallart Carme, Grand Robert, Fragkoudi Francesca, Pérez Isabel, Cassisi Santi, Fernández-Alvar Emma, Queiroz Anna B., Aznar-Menargues Guillem, González-Koda Yllari K., Rivero Alicia, Surot Francisco, Thomas Guillaume F., Bieri Rebekka, Gomez Facundo A., Pakmor Rüdiger, van de Voort Freeke
Natura: Artigo
Lingua:Inglês
Pubblicazione: EDP Sciences 2026-01-01
Serie:Astronomy & Astrophysics
Soggetti:
hertzsprung-russell and c-m diagrams
galaxy: disk
galaxy: evolution
solar neighborhood
galaxy: stellar content
Accesso online:https://www.aanda.org/articles/aa/full_html/2026/01/aa56468-25/aa56468-25.html
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