Browsing by Author "Few, C. G."

Browsing by Author "Few, C. G."

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    Chemodynamics of a simulated disc galaxy: initial mass functions and Type Ia supernova progenitors 
    Few, C. G.; Courty, S.; Gibson, Brad K.; Michel-Dansac, L.; Calura, F. (Oxford University Press, 2014-11-11)
    We trace the formation and advection of several elements within a cosmological adaptive mesh refinement simulation of an L★ galaxy. We use nine realizations of the same initial conditions with different stellar ...

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    The cold gas content of bulgeless dwarf galaxies 
    Pilkington, K.; Gibson, Brad K.; Calura, F.; Brooks, A. M.; Mayer, L.; Brook, C. B.; Stinson, G. S.; Thacker, Robert John, 1970-; Few, C. G.; Cunnama, D. (Wiley-Blackwell, 2011-11)
    We present an analysis of the neutral hydrogen (H I) properties of a fully cosmological hydrodynamical dwarf galaxy, run with varying simulation parameters. As reported by Governato et al., the high-resolution, high star ...

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    Metallicity gradients in disks: Do galaxies form inside-out? 
    Pilkington, K.; Few, C. G.; Gibson, Brad K.; Calura, F.; Michel-Dansac, L.; Thacker, Robert John, 1970-; Molla, M.; Matteucci, F.; Rahimi, A.; Kawata, D. (EDP Sciences, 2012-04)
    Aims. We examine radial and vertical metallicity gradients using a suite of disk galaxy hydrodynamical simulations, supplemented with two classic chemical evolution approaches. We determine the rate of change of gradient ...

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    Properties of simulated Milky Way-mass galaxies in loose group and field environments 
    Few, C. G.; Gibson, Brad K.; Courty, S.; Michel-Dansac, L.; Brook, C. B.; Stinson, G. S. (EDP Sciences, 2012-11)
    Aims. We test the validity of comparing simulated field disk galaxies with the empirical properties of systems situated within environments more comparable to loose groups, including the Milky Way’s Local Group. Methods. ...

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    RAMSES-CH: a new chemodynamical code for cosmological simulations 
    Gibson, Brad K.; Few, C. G.; Courty, S.; Kawata, D.; Calura, F.; Teyssier, R. (Oxford University Press on behalf of the Royal Astronomical Society, 2012-07)
    We present a new chemodynamical code – RAMSES-CH – for use in simulating the self-consistent evolution of chemical and hydrodynamical properties of galaxies within a fully cosmological framework. We build upon the adaptive ...

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    The stellar metallicity distribution of disc galaxies and bulges in cosmological simulations 
    Gibson, Brad K.; Calura, F.; Michel-Dansac, L.; Stinson, G. S.; Dotter, A.; Pilkington, K.; House, E. L.; Brook, C. B.; Few, C. G.; Cignoni, M. (Royal Astronomical Society, 2012-12)
    By means of high-resolution cosmological hydrodynamical simulations of Milky Way (MW) like disc galaxies, we conduct an analysis of the associated stellar metallicity distribution functions (MDFs). After undertaking a ...