DiRAC-3 Operations 2019-2022 - Cambridge [2020-06 resubmission]

Lead Research Organisation: University of Cambridge
Department Name: Institute of Astronomy

Abstract

DiRAC-3 Operations 2019-2022 resubmission; This is an administrative resubmission to replace ST/S003800/1 which has already been peer-reviewed.

Publications

10 25 50

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Borukhovetskaya A (2022) The tidal evolution of the Fornax dwarf spheroidal and its globular clusters in Monthly Notices of the Royal Astronomical Society

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Sawala T (2023) The timeless timing argument and the total mass of the Local Group in Monthly Notices of the Royal Astronomical Society: Letters

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Santos-Santos I (2023) The Tucana dwarf spheroidal: a distant backsplash galaxy of M31? in Monthly Notices of the Royal Astronomical Society

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Shao S (2021) The twisted dark matter halo of the Milky Way in Monthly Notices of the Royal Astronomical Society

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Falle S (2020) Thermal instability revisited in Monthly Notices of the Royal Astronomical Society

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Lawlor D (2022) Thermal Transitions in Dense Two-Colour QCD in EPJ Web of Conferences

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Trotta D (2023) Three-dimensional modelling of the shock-turbulence interaction in Monthly Notices of the Royal Astronomical Society

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Vanon R (2023) Three-dimensional Simulations of Massive Stars. II. Age Dependence in The Astrophysical Journal

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Pastorek A (2022) Time-resolved fourier transform infrared emission spectroscopy of NH radical in the X3S- ground state in Journal of Quantitative Spectroscopy and Radiative Transfer

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Cuesta-Lazaro C (2020) Towards a non-Gaussian model of redshift space distortions in Monthly Notices of the Royal Astronomical Society

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Brown S (2022) Towards a universal model for the density profiles of dark matter haloes in Monthly Notices of the Royal Astronomical Society

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Ruan C (2022) Towards an accurate model of small-scale redshift-space distortions in modified gravity in Monthly Notices of the Royal Astronomical Society

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Yurchenko SN (2020) Treating linear molecules in calculations of rotation-vibration spectra. in The Journal of chemical physics

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Panic O (2020) TW Hya: an old protoplanetary disc revived by its planet in Monthly Notices of the Royal Astronomical Society

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Le Saux A (2023) Two-dimensional simulations of internal gravity waves in a 5 M? zero-age-main-sequence model in Monthly Notices of the Royal Astronomical Society

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Eke V (2020) Understanding the large inferred Einstein radii of observed low-mass galaxy clusters in Monthly Notices of the Royal Astronomical Society

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Deason A (2023) Unravelling the mass spectrum of destroyed dwarf galaxies with the metallicity distribution function in Monthly Notices of the Royal Astronomical Society

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Wu Y (2023) Using planet migration and dust drift to weigh protoplanetary discs in Monthly Notices of the Royal Astronomical Society

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Robins L (2020) Viscous and inviscid strato-rotational instability in Journal of Fluid Mechanics

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Ryczanowski D (2020) What does strong gravitational lensing? The mass and redshift distribution of high-magnification lenses in Monthly Notices of the Royal Astronomical Society

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Pichon C (2020) Why do extremely massive disc galaxies exist today? in Monthly Notices of the Royal Astronomical Society

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Ramírez-Galeano L (2022) Why most molecular clouds are gravitationally dominated in Monthly Notices of the Royal Astronomical Society

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Robson D (2020) X-ray emission from hot gas in galaxy groups and clusters in simba in Monthly Notices of the Royal Astronomical Society