CS
Christine Simpson
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Galaxies: Formation, Evolution, Phenomena · Stellar, planetary, and galactic studies · Astrophysics and Star Formation Studies
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Publications (33)
- Auriga Streams III: the mass–metallicity relation does not rule out tidal mass-loss in Local Group satellites Save
- In-Transit Data Transport Strategies for Coupled AI-Simulation Workflow Patterns 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
- 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
- An ever-present Gaia snail shell triggered by a dark matter wake Save
- How cosmic rays mediate the evolution of the interstellar medium Save
- Colour and infall time distributions of satellite galaxies in simulated Milky-Way analogues Save
- Simulating radio synchrotron emission in star-forming galaxies: small-scale magnetic dynamo and the origin of the far-infrared–radio correlation Save
- Machine learning for galactic archaeology: a chemistry-based neural network method for identification of accreted disc stars Save
- Linking the brightest stellar streams with the accretion history of Milky Way like galaxies Save
- Formation and fate of low-metallicity stars in TNG50 Save
- Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation Save
- Satellites around Milky Way Analogs: Tension in the Number and Fraction of Quiescent Satellites Seen in Observations versus Simulations Save
- A tale of two populations: surviving and destroyed dwarf galaxies and the build-up of the Milky Way’s stellar halo Save
- Magnetizing the circumgalactic medium of disc galaxies Save
- The edge of the Galaxy Save
- The milky way total mass profile as inferred from Gaia DR2 Save
- Efficacy of early stellar feedback in low gas surface density environments Save