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Field of Research : Galactic Astronomy
Status : Active
Research Topic : FOLLICLE FLUID
Australian State/Territory : VIC
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  • Active Funded Activity

    ARC Future Fellowships - Grant ID: FT160100046

    Funder
    Australian Research Council
    Funding Amount
    $651,000.00
    Summary
    The convective boundaries in stars. This project aims to locate the boundaries of convection, a problem in models of stars. It will calculate high-resolution three-dimensional simulations of stars and observe star clusters. The effect of this advance on stellar modelling could be profound since almost all stars contain convective regions. Many branches of astronomy rely on stellar models so the effect could extend far beyond the immediate field, ultimately expanding understanding of the Universe .... The convective boundaries in stars. This project aims to locate the boundaries of convection, a problem in models of stars. It will calculate high-resolution three-dimensional simulations of stars and observe star clusters. The effect of this advance on stellar modelling could be profound since almost all stars contain convective regions. Many branches of astronomy rely on stellar models so the effect could extend far beyond the immediate field, ultimately expanding understanding of the Universe. It could also be crucial in realising the scientific advances of the surveys which are gathering data for up to a billion stars.
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    Active Funded Activity

    Discovery Projects - Grant ID: DP190102431

    Funder
    Australian Research Council
    Funding Amount
    $386,660.00
    Summary
    Nucleosynthetic signatures of convective-reactive events in stars. This project aims to better understand where the elements in the periodic table come from, by investigating spectacular but poorly understood nuclear-burning events that occur in stars. The project aims to understand the inner workings of stars by calculating detailed three-dimensional simulations using Australia's largest supercomputers, and to combine this with telescope surveys that are recording the chemical make-up of millio .... Nucleosynthetic signatures of convective-reactive events in stars. This project aims to better understand where the elements in the periodic table come from, by investigating spectacular but poorly understood nuclear-burning events that occur in stars. The project aims to understand the inner workings of stars by calculating detailed three-dimensional simulations using Australia's largest supercomputers, and to combine this with telescope surveys that are recording the chemical make-up of millions of stars. The project expects to create new knowledge in the areas of stellar physics and nucleosynthesis. Many branches of astronomy rely on stellar models so the impact would extend far beyond the immediate field, ultimately expanding our understanding of the Universe.
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