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NON-STANDARD STRUCTURE FORMATION SCENARIOS.
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- Astrophysics & Space Science, 2003, v. 284, n. 2, p. 335, doi. 10.1023/A:1024021908845
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The stellar halo in Local Group Hestia simulations: III. Chemical abundance relations for accreted and in situ stars.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 677, p. 1, doi. 10.1051/0004-6361/202244234
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- Article
The stellar halo in Local Group Hestia simulations: II. The accreted component.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 677, p. 1, doi. 10.1051/0004-6361/202244233
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- Article
The stellar halo in Local Group Hestia simulations: I. The in situ component and the effect of mergers.
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- Astronomy & Astrophysics / Astronomie et Astrophysique, 2023, v. 677, p. 1, doi. 10.1051/0004-6361/202244232
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- Article
The dynamics of cluster substructure.
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- Proceedings of the International Astronomical Union, 2004, v. 2004, n. IAUC195, p. 280, doi. 10.1017/S1743921304000596
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- Article
Cold versus Warm Dark Matter Simulations of a Galaxy Group.
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- Publications of the Astronomical Society of Australia, 2013, v. 30, p. 1, doi. 10.1017/pasa.2013.16
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- Article