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Uncovering the birth of the Milky Way through accurate stellar ages with Gaia
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“As Gallart et al. (2019) showed, the majority of the thick disk stars likely formed during/after the merger with Gaia-Enceladus and not before.”
From Streams, Substructures, and the Early History of the Milky Way (2020) · cites this paper as Gallart et al. (2019)
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“2018) suggest a mass ratio of ∼4:1 for the merger (which has been confirmed by Gallart et al. 2019) on the basis of the estimated stellar mass of Gaia-Enceladus, the expected stellar mass-to-halo mass ratio for objects of this size, and the assumption that a 10 10 M ࣻ thick disk stellar mass is present at the time.”
From Streams, Substructures, and the Early History of the Milky Way (2020) · cites this paper as Gallart et al. 2019
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“The evidence discussed above, particularly the work of Gallart et al. (2019), supports a scenario in which a gas-rich disk experienced a merger with Gaia-Enceladus, where the stars already present were dynamically heated, and star formation was triggered (possibly in a starburst), leading to the formation of the bulk of the stars in the thick disk.”
From Streams, Substructures, and the Early History of the Milky Way (2020) · cites this paper as Gallart et al. (2019)
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“Helmi et al. (2018) suggest a mass ratio of ∼4:1 for the merger (which has been confirmed byGallart et al. 2019) on the basis of the estimated stellar mass of Gaia-Enceladus, the expected stellar mass-to-halo mass ratio for objects of this size, and the assumption that a 10 10 M ࣻ thick disk stellar mass is present at the time.”
From Streams, Substructures, and the Early History of the Milky Way (2020) · cites this paper as Gallart et al. 2019
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The age structure of the Milky Way’s halo
Carollo, D., Beers, T. C., Placco, V. M., Santucci, R. M., Denissenkov, P. A., Tissera, P. B., Lentner, G., Rossi, S., Lee, Y. S., & Tumlinson, J. (2016) · Nature Physics · doi:10.1038/nphys3874 · Cited by 45
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Origin of the metallicity distribution in the thick disc
Miranda, M., Pilkington, K., Gibson, B. K., Brook, C. B., Sánchez–Blázquez, P., Minchev, I., Few, C. G., Smith, R., Domínguez-Tenreiro, R., Obreja, A., et al. (2015) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201525789 · Cited by 37
Self-citationThe central spheroids of Milky Way mass-sized galaxies
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Integrated-light analyses vs. colour-magnitude diagrams
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Self-citation
Metadata
- Authors
- Gallart, C., Bernard, E. J., Brook, C. B., Ruiz-Lara, T., Cassisi, S., Hill, V., & Monelli, M.
- Affiliations
- Universidad de La Laguna (ES)
- Centre National de la Recherche Scientifique (FR)
- Collurania Teramo Observatory (IT)
- Corresponding author
- Gallart, Carme
- ORCID
- Venue
- Nature Astronomy
- Published
- 2019-07-22
- Volume
- 3
- Issue
- 10
- Pages
- 932-939
- ISSN
- 2397-3366 (ISSN-L)
- OpenAlex
- W2963416706
- Cited by
- 262
- References
- 102
- Citations by year
- 2026: 21 · 2025: 35 · 2024: 36 · 2023: 45 · 2022: 30 · 2021: 47 · 2020: 36 · 2019: 12
- FWCI
- 16.68
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Licence
- Locations
- Nature Astronomy (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- HAL (submittedVersion, cc-by)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Keywords
- Milky Way formation, stellar ages, Gaia-Enceladus, Gaia, Galactic halo, thick disk, galaxy mergers, stellar kinematics, galaxy accretion
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