Publications (46) Arianna Di Cintio publications

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2025

  1. A physically motivated galaxy size definition across different state-of-the-art hydrodynamical simulations

    Astronomy and Astrophysics, Vol. 699

  2. Are Gas-rich Ultra-diffuse Galaxies and Field Dwarfs Distinct?

    Astrophysical Journal, Vol. 989, Núm. 1

2024

  1. The role of active galactic nucleus feedback on the evolution of dwarf galaxies from cosmological simulations: Supermassive black holes suppress star formation in low-mass galaxies

    Astronomy and Astrophysics, Vol. 690

2023

  1. 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

  2. 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

  3. Metallicity profiles of ultradiffuse galaxies in NIHAO simulations

    Monthly Notices of the Royal Astronomical Society, Vol. 519, Núm. 1, pp. 1545-1561

  4. On the anticorrelation between pericentric distance and inner dark matter density of Milky Way’s dwarf spheroidal galaxies

    Monthly Notices of the Royal Astronomical Society, Vol. 522, Núm. 2, pp. 3058-3066

  5. The Undiscovered Ultradiffuse Galaxies of the Local Group

    Astrophysical Journal Letters, Vol. 946, Núm. 2

2021

  1. 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

  2. Origin of stellar prolate rotation in a cosmologically simulated faint dwarf galaxy

    Monthly Notices of the Royal Astronomical Society: Letters, Vol. 505, Núm. 1, pp. L100-L105

  3. Pericentric passage-driven star formation in satellite galaxies and their hosts: CLUES from local group simulations

    Monthly Notices of the Royal Astronomical Society, Vol. 506, Núm. 1, pp. 531-545

2020

  1. 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

  2. Self-interacting dark matter and the delay of supermassive black hole growth

    Monthly Notices of the Royal Astronomical Society, Vol. 500, Núm. 2, pp. 2177-2187

  3. 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

  1. A distance of 13 mpc resolves the claimed anomalies of the galaxy lacking dark matter

    Monthly Notices of the Royal Astronomical Society, Vol. 486, Núm. 1, pp. 1-31

  2. Dark matter response to galaxy assembly history

    Astronomy and Astrophysics, Vol. 622

  3. Erratum: NIHAO IV: Core creation and destruction in dark matter density profiles across cosmic time (Monthly Notices of the Royal Astronomical Society DOI: 10.1093/mnras/stv2856)

    Monthly Notices of the Royal Astronomical Society

  4. Formation of ultra-diffuse galaxies in the field and in galaxy groups

    Monthly Notices of the Royal Astronomical Society, Vol. 487, Núm. 4, pp. 5272-5290

  5. Full-spectral fitting techniques to characterise the stellar content of ultra diffuse galaxies

    Proceedings of the International Astronomical Union

  6. NIHAO XXI: The emergence of low surface brightness galaxies

    Monthly Notices of the Royal Astronomical Society, Vol. 486, Núm. 2, pp. 2535-2548