The DOI matches its Crossref record; 70 of the 70 references it cites were found in a registry or an index.
Two stellar components in the halo of the Milky Way
Open accessAbstract
The halo of the Milky Way provides unique elemental abundance and kinematic information on the first objects to form in the Universe, and this information can be used to tightly constrain models of galaxy formation and evolution. Although the halo was once considered a single component, evidence for its dichotomy has slowly emerged in recent years from inspection of small samples of halo objects. Here we show that the halo is indeed clearly divisible into two broadly overlapping structural components--an inner and an outer halo--that exhibit different spatial density profiles, stellar orbits and stellar metallicities (abundances of elements heavier than helium). The inner halo has a modest net prograde rotation, whereas the outer halo exhibits a net retrograde rotation and a peak metallicity one-third that of the inner halo. These properties indicate that the individual halo components probably formed in fundamentally different ways, through successive dissipational (inner) and dissipationless (outer) mergers and tidal disruption of proto-Galactic clumps.
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“There is, however, still some tension with the work of Carollo et al. (2007) because what they called the outer halo peaked at a metallicity of [Fe/H] ∼ -2.2, lower than is typical for Gaia-Enceladus stars.”
From Streams, Substructures, and the Early History of the Milky Way (2020) · cites this paper as Carollo et al. 2007
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Schlegel, D. J., Finkbeiner, D. P., & Davis, M. (1998) · The Astrophysical Journal · doi:10.1086/305772 · Cited by 15,126
The Sloan Digital Sky Survey: Technical Summary
York, D., Adelman, J., Anderson, J., Anderson, S., Annis, J., Bahcall, N., Bakken, J., Barkhouser, R., Bastian, S., Berman, E., et al. (2000) · The Astronomical Journal · doi:10.1086/301513 · Cited by 8,368
Self-citationCore condensation in heavy halos: a two-stage theory for galaxy formation and clustering
White, S. D. M., & Rees, M. J. (1978) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/183.3.341 · Cited by 3,919
The Sloan Digital Sky Survey Photometric System
Fukugita, M., Ichikawa, T., Gunn, J. E., Doi, M., Shimasaku, K., & Schneider, D. P. (1996) · The Astronomical Journal · doi:10.1086/117915 · Cited by 3,033
Sloan Digital Sky Survey: Early Data Release
Stoughton, C., Lupton, R. H., Bernardi, M., Blanton, M. R., Burles, S. M., Castander, F. J., Connolly, A. J., Eisenstein, D. J., Frieman, J. A., Hennessy, G. S., et al. (2002) · The Astronomical Journal · doi:10.1086/324741 · Cited by 2,389
Self-citationThe 2.5 m Telescope of the Sloan Digital Sky Survey
Gunn, J. E., Siegmund, W. A., Mannery, E. J., Owen, R. E., Hull, C. L., Leger, R. F., Carey, L. N., Knapp, G. R., York, D. G., Boroski, W. N., et al. (2006) · The Astronomical Journal · doi:10.1086/500975 · Cited by 2,373
Self-citationThe Sloan Digital Sky Survey Photometric Camera
Gunn, J. E., Carr, M., Rockosi, C., Sekiguchi, M., Berry, K., Elms, B., de Haas, E., Ivezić, Ž., Knapp, G., Lupton, R., et al. (1998) · The Astronomical Journal · doi:10.1086/300645 · Cited by 1,692
Self-citationEvidence from the motions of old stars that the Galaxy collapsed.
Eggen, O. J., Donald Lynden-bell, A., & Sandage, A. (1962) · The Astrophysical Journal · doi:10.1086/147433 · Cited by 1,665
Compositions of halo clusters and the formation of the galactic halo
Searle, L., & Zinn, R. (1978) · The Astrophysical Journal · doi:10.1086/156499 · Cited by 1,524
The Field of Streams: Sagittarius and Its Siblings
Belokurov, V. A., Zucker, D. B., Evans, N. W., Gilmore, G. F., Vidrih, S., Bramich, D. M., Newberg, H. J., Wyse, R. F. Ġ., Irwin, M. J., Fellhauer, M., et al. (2006) · The Astrophysical Journal · doi:10.1086/504797 · Cited by 910
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Stellar halos of bright central galaxies
Contini, E., Spavone, M., Ragusa, R., Iodice, E., & Yi, S. K. (2026) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202557921
Stellar Populations in the Extreme Outer Halo of the Spiral Galaxy M96
Mihos, J. C., Durrell, P. R., Malkan, B. K., & Watkins, A. E. (2026) · The Astrophysical Journal · doi:10.3847/1538-4357/ae3fa2
Testing the chemical tagging technique with open clusters
Blanco-Cuaresma, S. (2014) · doi:10.70675/5a394d0dz1b47z427bz926fz5eb9e50a2cbd
Thomas, G. F. (2017) · theses.fr (ABES) · doi:10.70675/ec81075ez0b76z41adzb34dza930cf69d154
Galactic archaeology of the Milky Way disc with the Gaia space mission
Santos-Peral, P. (2021) · theses.fr (ABES) · doi:10.70675/a51ab6eazf94dz4aa0z91dczb6fc6b1d07cc
Symbolic machine learning for physics and astrophysics
Tenachi, W. (2024) · theses.fr (ABES) · doi:10.70675/21d89f84z0086z44f7z94c9z91f2716779a2
The Milky Way tomography with Subaru Hyper Suprime-Cam. II. Smooth halo structure
Suzuki, Y., Chiba, M., Wyse, R. F. Ġ., & Horigome, S.-I. (2026) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psag149
Self-citationCharacterizing the Velocity Anisotropy of the Milky Way’s Stellar Halo
Barbosa, F. O., Pérez-Villegas, Á., Rossi, S., Santucci, R. M., Aguilar, L., Perottoni, H. D., Limberg, G., Borbolato, L., & Nogueira-Santos, J. V. (2026) · The Astrophysical Journal · doi:10.3847/1538-4357/ae8fd6
The dynamics of old inner galaxy stars in Milky Way-mass galaxies using FIRE-2 simulations
Tasso, E., Lucey, M., Sanderson, R. E., Kundu, A., & Necib, L. (2026) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stag1139
Metadata
- Authors
- Carollo, D., Beers, T. C., Lee, Y. S., Chiba, M., Norris, J. E., Wilhelm, R., Sivarani, T., Marsteller, B., Munn, J. A., Bailer-Jones, C. A. L., Fiorentin, P. R., & York, D. G.
- Affiliations
- Osservatorio Astrofisico di Torino (IT)
- Joint Institute for Nuclear Astrophysics (US)
- Tohoku University (JP)
- Australian National University (AU)
- Texas Tech University (US)
- United States Naval Observatory (US)
- University of Ljubljana (SI)
- University of Chicago (US)
- Corresponding author
- Carollo, Daniela
- ORCID
- Venue
- Nature
- Published
- 2007-12-13
- Volume
- 450
- Issue
- 7172
- Pages
- 1020-1025
- ISSN
- 0028-0836 (ISSN-L)
- 1476-4687
- OpenAlex
- W2088048947
- Cited by
- 626
- References
- 70
- Citations by year
- 2026: 7 · 2025: 8 · 2024: 17 · 2023: 18 · 2022: 14 · 2021: 32 · 2020: 37 · 2019: 40 · 2018: 43 · 2017: 29 · 2016: 48 · 2015: 32 · 2014: 30 · 2013: 34 · 2012: 46
- FWCI
- 30.32
- Type
- journal article
- Language
- en
- Update notices
- erratum (2008-01-10)
- Open access
- green
- arxiv.org
- Locations
- Nature (publishedVersion)
- arXiv (Cornell University) (publishedVersion)
- PubMed (publishedVersion)
- ANU Open Research (Australian National University) (submittedVersion)
- Defense Technical Information Center (DTIC) (submittedVersion)
- RePEc: Research Papers in Economics (submittedVersion)
- Max Planck Institute for Plasma Physics (submittedVersion)
- 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
- Galactic halo, inner halo, outer halo, stellar metallicity, stellar rotation, stellar orbits, dissipationless mergers, tidal disruption, galaxy formation, stellar populations
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