Christopher Bryan Anderson
Brook
Profesor Contratado Doctor
Instituto de Astrofísica de Canarias
Santa Cruz de Tenerife, EspañaPublikationen in Zusammenarbeit mit Forschern von Instituto de Astrofísica de Canarias (23)
2023
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A high fidelity Milky Way simulation with Kraken, Gaia-Enceladus, and Sequoia analogues: clues to their accretion histories
Monthly Notices of the Royal Astronomical Society, Vol. 526, Núm. 1, pp. 1190-1197
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A probabilistic deep learning model to distinguish cusps and cores in dwarf galaxies
Monthly Notices of the Royal Astronomical Society, Vol. 519, Núm. 3, pp. 4384-4396
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Constraining gas metal mixing strength in simulations using observations of the Milky Way's disc
Monthly Notices of the Royal Astronomical Society, Vol. 525, Núm. 1, pp. 279-285
2021
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A Shallow Dark Matter Halo in Ultra-diffuse Galaxy AGC 242019: Are UDGs Structurally Similar to Low-surface-brightness Galaxies?
Astrophysical Journal Letters, Vol. 919, Núm. 1
2020
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Explaining the chemical trajectories of accreted and in-situ halo stars of the Milky Way
Monthly Notices of the Royal Astronomical Society, Vol. 495, Núm. 3, pp. 2645-2651
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NIHAO XXIV: rotation- or pressure-supported systems? Simulated Ultra Diffuse Galaxies show a broad distribution in their stellar kinematics
Monthly Notices of the Royal Astronomical Society, Vol. 497, Núm. 4, pp. 4282-4292
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The mass of our Galaxy from satellite proper motions in the Gaia era
Monthly Notices of the Royal Astronomical Society, Vol. 494, Núm. 4, pp. 5178-5193
2019
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NIHAO XXI: The emergence of low surface brightness galaxies
Monthly Notices of the Royal Astronomical Society, Vol. 486, Núm. 2, pp. 2535-2548
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Uncovering the birth of the Milky Way through accurate stellar ages with Gaia
Nature Astronomy
2018
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CLUES about M33: The reversed radial stellar age gradient in the outskirts of Triangulum galaxy
Monthly Notices of the Royal Astronomical Society, Vol. 480, Núm. 4, pp. 4455-4467
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Gaia DR2 proper motions of dwarf galaxies within 420 kpc: Orbits, Milky Way mass, tidal influences, planar alignments, and group infall
Astronomy and Astrophysics, Vol. 619
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Metallicity gradient of the thick disc progenitor at high redshift
Monthly Notices of the Royal Astronomical Society, Vol. 473, Núm. 1, pp. 867-878
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NIHAO - XIV. Reproducing the observed diversity of dwarf galaxy rotation curve shapes in ΛCDM
Monthly Notices of the Royal Astronomical Society, Vol. 473, Núm. 4, pp. 4392-4403
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On the early evolution of Local Group dwarf galaxy types: Star formation and supernova feedback
Monthly Notices of the Royal Astronomical Society, Vol. 479, Núm. 2, pp. 1514-1527
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Spectroscopic characterization of the stellar content of ultra-diffuse galaxies
Monthly Notices of the Royal Astronomical Society, Vol. 478, Núm. 2, pp. 2034-2045
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Stellar feedback and the energy budget of late-type Galaxies: Missing baryons and core creation
Monthly Notices of the Royal Astronomical Society, Vol. 480, Núm. 4, pp. 4287-4301
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Ultra-Diffuse Galaxies: A formation scenario
Proceedings of the 13th Scientific Meeting of the Spanish Astronomical Society - Highlights of Spanish Astrophysics X, SEA 2018
2017
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Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
Astronomy and Astrophysics, Vol. 603
2011
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A comparison of galaxy group luminosity functions from semi-analytic models
Monthly Notices of the Royal Astronomical Society, Vol. 415, Núm. 3, pp. 2798-2811
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Metallicity gradients of disc stars for a cosmologically simulated galaxy
Monthly Notices of the Royal Astronomical Society, Vol. 415, Núm. 2, pp. 1469-1478