FG
Facundo Ariel Gomez
University of La Serena, Max Planck Society, University of Groningen, Universidad Nacional de La Plata Facultad de Ciencias Astronómicas y Geofísicas, Michigan State University
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Galaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
0000-0003-4232-8584
Employment
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Universidad de La Serena Associate Professor2017 - Present
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Max Planck Society Fixed term staff2014 - 2017
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Michigan State University Research Associate2010 - 2014
Education
- ? - 2010
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Universidad Nacional de La Plata Facultad de Ciencias Astronómicas y Geofísicas? - 2006
Projects & Funding
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The remnants of galaxies: characterising disrupted dwarf galaxies and stripped nuclei in the halo of Milky Way mass galaxies Agencia Nacional de Investigación y Desarrollo2025 - 2027
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The giants glow: characterizing the formation of the intra cluster light Agencia Nacional de Investigación y Desarrollo2022 - 2024
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The Drums of Growth: What paces galaxy evolution? Agencia Nacional de Investigación y Desarrollo2021 - 2025
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The Formation and Evolution of Milky Way-like galaxies Agencia Nacional de Investigación y Desarrollo2018 - 2020
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MPA - ULS Partner Group Max Planck Society2018 - 2024
Publications (141)
- Characterising the formation and evolution of S0-galaxies (CaFES-0): Their formation pathways around galaxy clusters Save
- Coupling between stellar and HI lopsidedness in Milky Way–type galaxies from the Auriga Superstars cosmological simulations Save
- Something green beneath the surface: The dynamical nature of fossil structures in IllustrisTNG-100 Save
- X-ray emission maps and scaling relations in IllustrisTNG and MillenniumTNG Save
- Characterising the formation and evolution of S0-galaxies (CaFES-0): Revealing the origin of the mass-size relation of S0 galaxies Save
- Age and metallicity of low-mass galaxies: From their centres to their stellar halos Save
- Stirring things up: Bar-induced substructures in the stellar halo of a cosmological Milky Way analogue Save
- The diverse nature of spiral arms in the auriga Superstars cosmological hydrodynamic simulations Save
- Coevolution of intracluster light and brightest cluster galaxies Save
- Origins of coplanar counterrotating stellar disk components in late-type galaxies Save
- Auriga Streams III: the mass–metallicity relation does not rule out tidal mass-loss in Local Group satellites Save
- Stream automatic detection with convolutional neural networks Save
- Auriga Superstars: Improving the resolution and fidelity of stellar dynamics in cosmological galaxy simulations Save
- Quantifying the intrinsic variability due to randomness of the Auriga galaxy formation model Save
- The distribution and origin of metals in simulated Milky Way-like galaxies Save
- Auriga Streams – I: disrupting satellites surrounding Milky Way-mass haloes at multiple resolutions Save
- Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies Save
- A statistical study of lopsided galaxies using random forests Save
- Differences in the physical properties of satellite galaxies within relaxed and disturbed galaxy groups and clusters Save
- The formation and evolution of supermassive disks in IllustrisTNG Save