DiRAC Bridging Grant 2019 - Cambridge
Lead Research Organisation:
University of Cambridge
Department Name: Institute of Astronomy
Abstract
Abstracts are not currently available in GtR for all funded research. This is normally because the abstract was not required at the time of proposal submission, but may be because it included sensitive information such as personal details.
Organisations
Publications
Vidal J
(2020)
Efficiency of tidal dissipation in slowly rotating fully convective stars or planets
in Monthly Notices of the Royal Astronomical Society
Vidal J
(2020)
Turbulent Viscosity Acting on the Equilibrium Tidal Flow in Convective Stars
in The Astrophysical Journal Letters
Vidal J
(2020)
Turbulent Viscosity Acting on the Equilibrium Tidal Flow in Convective Stars
in The Astrophysical Journal Letters
Vera-Casanova A
(2022)
Linking the brightest stellar streams with the accretion history of Milky Way like galaxies
in Monthly Notices of the Royal Astronomical Society
Varghese A
(2023)
Chemical Mixing Induced by Internal Gravity Waves in Intermediate-mass Stars
in The Astrophysical Journal
Varghese A
(2024)
Effect of Rotation on Wave Mixing in Intermediate-mass Stars
in The Astrophysical Journal
Van Son L
(2019)
Galaxies with monstrous black holes in galaxy cluster environments
in Monthly Notices of the Royal Astronomical Society
Van Loon M
(2021)
Explaining the scatter in the galaxy mass-metallicity relation with gas flows
in Monthly Notices of the Royal Astronomical Society
Van Daalen M
(2020)
Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
in Monthly Notices of the Royal Astronomical Society
Vanon R
(2023)
Three-dimensional Simulations of Massive Stars. II. Age Dependence
in The Astrophysical Journal
Vandenbroucke B
(2021)
Polarised emission from aligned dust grains in nearby galaxies: Predictions from the Auriga simulations
in Astronomy & Astrophysics
Vandenbroucke B
(2019)
Radiation hydrodynamics simulations of the evolution of the diffuse ionized gas in disc galaxies
in Monthly Notices of the Royal Astronomical Society
Vandenbroucke B
(2020)
CMACIONIZE 2.0: a novel task-based approach to Monte Carlo radiation transfer
in Astronomy & Astrophysics
Vandenbroucke B
(2020)
Infrared luminosity functions and dust mass functions in the EAGLE simulation
in Monthly Notices of the Royal Astronomical Society
Vandenbroucke B
(2019)
Testing the stability of supersonic ionized Bondi accretion flows with radiation hydrodynamics
in Monthly Notices of the Royal Astronomical Society
Upadhye A
(2024)
Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations versus fast approximations
in Monthly Notices of the Royal Astronomical Society
Upadhyay A
(2021)
Star formation histories of Coma cluster galaxies matched to simulated orbits hint at quenching around first pericenter
in Astronomy & Astrophysics
Turpin G
(2024)
Orbital evolution of close binary systems: comparing viscous and wind-driven circumbinary disc models
in Monthly Notices of the Royal Astronomical Society
Tsang Y
(2020)
Characterising Jupiter's dynamo radius using its magnetic energy spectrum
in Earth and Planetary Science Letters
Tsang Y
(2020)
Characterising Jupiter's dynamo radius using its magnetic energy spectrum
in Earth and Planetary Science Letters
Tsang Y
(2024)
Scaling of the geomagnetic secular variation timescale
in Geophysical Journal International
Tröster T
(2019)
Painting with baryons: augmenting N -body simulations with gas using deep generative models
in Monthly Notices of the Royal Astronomical Society: Letters
Trusov S
(2024)
The two-point correlation function covariance with fewer mocks
in Monthly Notices of the Royal Astronomical Society
Trujillo-Gomez S
(2023)
In situ or accreted? Using deep learning to infer the origin of extragalactic globular clusters from observables
in Monthly Notices of the Royal Astronomical Society
Trujillo-Gomez S
(2021)
The kinematics of globular cluster populations in the E-MOSAICS simulations and their implications for the assembly history of the Milky Way
in Monthly Notices of the Royal Astronomical Society
Trotta D
(2020)
Fast Acceleration of Transrelativistic Electrons in Astrophysical Turbulence
in The Astrophysical Journal
Trotta D
(2023)
Three-dimensional modelling of the shock-turbulence interaction
in Monthly Notices of the Royal Astronomical Society
Trotta D
(2022)
Single-spacecraft techniques for shock parameters estimation: A systematic approach
in Frontiers in Astronomy and Space Sciences
Trotta D
(2022)
On the Transmission of Turbulent Structures across the Earth's Bow Shock
in The Astrophysical Journal
Trotta D
(2023)
Irregular Proton Injection to High Energies at Interplanetary Shocks
in The Astrophysical Journal Letters
Tripathi B
(2024)
Predicting the Slowing of Stellar Differential Rotation by Instability-driven Turbulence
in The Astrophysical Journal
Tress R
(2020)
Simulations of the star-forming molecular gas in an interacting M51-like galaxy
in Monthly Notices of the Royal Astronomical Society
Tress R
(2020)
Simulations of the star-forming molecular gas in an interacting M51-like galaxy
in Monthly Notices of the Royal Astronomical Society
Tress R
(2020)
Simulations of the Milky Way's central molecular zone - I. Gas dynamics
in Monthly Notices of the Royal Astronomical Society
Trayford J
(2019)
Resolved galaxy scaling relations in the eagle simulation: star formation, metallicity, and stellar mass on kpc scales
in Monthly Notices of the Royal Astronomical Society
Trayford J
(2020)
Fade to grey: systematic variation of galaxy attenuation curves with galaxy properties in the eagle simulations
in Monthly Notices of the Royal Astronomical Society
Trayford J
(2019)
The star formation rate and stellar content contributions of morphological components in the EAGLE simulations
in Monthly Notices of the Royal Astronomical Society
Trayford J
(2020)
Massive low-surface-brightness galaxies in the eagle simulation
in Monthly Notices of the Royal Astronomical Society
Towler I
(2024)
Inferring the dark matter splashback radius from cluster gas and observable profiles in the FLAMINGO simulations
in Monthly Notices of the Royal Astronomical Society
Towler I
(2023)
Gas clumping and its effect on hydrostatic bias in the MACSIS simulations
in Monthly Notices of the Royal Astronomical Society
Tobias S
(2020)
Angular momentum transport, layering, and zonal jet formation by the GSF instability: non-linear simulations at a general latitude
in Monthly Notices of the Royal Astronomical Society
Tissera P
(2022)
The evolution of the oxygen abundance gradients in star-forming galaxies in the eagle simulations
in Monthly Notices of the Royal Astronomical Society
Tinoco-Arenas A
(2022)
Parametric Study of Magnetosheath Jets in 2D Local Hybrid Simulations
in Frontiers in Astronomy and Space Sciences
Tillman M
(2023)
Efficient Long-range Active Galactic Nuclei (AGNs) Feedback Affects the Low-redshift Lya Forest
in The Astrophysical Journal Letters
Threlfall J
(2020)
How Is Helicity (and Twist) Partitioned in Magnetohydrodynamic Simulations of Reconnecting Magnetic Flux Tubes?
in The Astrophysical Journal
Thompson O
(2024)
Predictions for CO emission and the CO-to-H2 conversion factor in galaxy simulations with non-equilibrium chemistry
in Monthly Notices of the Royal Astronomical Society
Thompson J
(2024)
Phenomenological gravitational-wave model for precessing black-hole binaries with higher multipoles and asymmetries
in Physical Review D
Thomas P
(2023)
First light and reionization epoch simulations ( Flares ) X: environmental galaxy bias and survey variance at high redshift
in Monthly Notices of the Royal Astronomical Society
Thomas N
(2019)
Black hole - Galaxy correlations in simba
in Monthly Notices of the Royal Astronomical Society
Thomas N
(2022)
The environments of the radio galaxy population in simba.
in Monthly notices of the Royal Astronomical Society
| Description | Many new discoveries about the formation and evolution of galaxies, star formation, planet formation and particle physics theory have been made possible by the award. |
| Exploitation Route | Many international collaborative projects are supported by the HPC resources provided by DiRAC. |
| Sectors | Aerospace Defence and Marine Creative Economy Digital/Communication/Information Technologies (including Software) Education Healthcare |