Search Results - "Georgy, C."
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The effects of surface fossil magnetic fields on massive star evolution: I. Magnetic field evolution, mass-loss quenching, and magnetic braking
Published in Monthly notices of the Royal Astronomical Society (01-06-2019)“…Abstract Surface magnetic fields have a strong impact on stellar mass loss and rotation and, as a consequence, on the evolution of massive stars. In this work,…”
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Dependence of convective boundary mixing on boundary properties and turbulence strength
Published in Monthly notices of the Royal Astronomical Society (21-04-2019)“…Abstract Convective boundary mixing is one of the major uncertainties in stellar evolution. In order to study its dependence on boundary properties and…”
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Apparent age spreads in clusters and the role of stellar rotation
Published in Monthly notices of the Royal Astronomical Society (21-10-2015)“…We use the Geneva syclist isochrone models that include the effects of stellar rotation to investigate the role that rotation has on the resulting…”
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3D hydrodynamic simulations of carbon burning in massive stars
Published in Monthly notices of the Royal Astronomical Society (11-10-2017)“…Abstract We present the first detailed 3D hydrodynamic implicit large eddy simulations of turbulent convection of carbon burning in massive stars. Simulations…”
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Extended main sequence turnoffs in open clusters as seen by Gaia – I. NGC 2818 and the role of stellar rotation
Published in Monthly notices of the Royal Astronomical Society (01-11-2018)Get full text
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A high fraction of Be stars in young massive clusters: evidence for a large population of near-critically rotating stars
Published in Monthly notices of the Royal Astronomical Society (11-03-2017)“…Recent photometric analyses of the colour-magnitude diagrams of young massive clusters (YMCs) have found evidence for splitting in the main sequence and…”
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Convective core entrainment in 1D main-sequence stellar models
Published in Monthly notices of the Royal Astronomical Society (01-05-2021)“…ABSTRACT 3D hydrodynamics models of deep stellar convection exhibit turbulent entrainment at the convective-radiative boundary which follows the entrainment…”
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The effects of surface fossil magnetic fields on massive star evolution – II. Implementation of magnetic braking in mesa and implications for the evolution of surface rotation in OB stars
Published in Monthly notices of the Royal Astronomical Society (01-03-2020)“…ABSTRACT The time evolution of angular momentum and surface rotation of massive stars are strongly influenced by fossil magnetic fields via magnetic braking…”
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The life cycles of Be viscous decretion discs: fundamental disc parameters of 54 SMC Be stars
Published in Monthly notices of the Royal Astronomical Society (21-05-2018)“…Abstract Be stars are main-sequence massive stars with emission features in their spectrum, which originates in circumstellar gaseous discs. Even though the…”
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The effects of stellar rotation along the main sequence of the 100-Myr-old massive cluster NGC 1850
Published in Monthly notices of the Royal Astronomical Society (01-01-2023)“…ABSTRACT Young star clusters enable us to study the effects of stellar rotation on an ensemble of stars of the same age and across a wide range in stellar mass…”
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3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star
Published in Monthly notices of the Royal Astronomical Society (30-05-2023)“…ABSTRACT Our knowledge of stellar evolution is driven by one-dimensional (1D) simulations. 1D models, however, are severely limited by uncertainties on the…”
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Did the progenitor of SN 2011dh have a binary companion?
Published in Monthly notices of the Royal Astronomical Society (11-12-2015)“…We present late-time Hubble Space Telescope ultraviolet (UV) and optical observations of the site of SN 2011dh in the galaxy M51, ∼1164 days post-explosion…”
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How stellar rotation shapes the colour−magnitude diagram of the massive intermediate-age star cluster NGC 1846
Published in Monthly notices of the Royal Astronomical Society (01-02-2020)“…ABSTRACT We present a detailed study of stellar rotation in the massive 1.5 Gyr old cluster NGC 1846 in the Large Magellanic Cloud. Similar to other clusters…”
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Shell mergers in the late stages of massive star evolution: new insight from 3D hydrodynamic simulations
Published in Monthly notices of the Royal Astronomical Society (01-09-2024)“…ABSTRACT One-dimensional (1D) stellar evolution models are widely used across various astrophysical fields, however they are still dominated by important…”
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Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
Published in Monthly notices of the Royal Astronomical Society (09-08-2022)“…ABSTRACT Our understanding of stellar structure and evolution coming from one-dimensional (1D) stellar models is limited by uncertainties related to…”
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The Effects of Surface Fossil Magnetic Fields on Massive Star Evolution: IV. Grids of Models at Solar, LMC, and SMC Metallicities
Published in Monthly notices of the Royal Astronomical Society (18-10-2022)“…Magnetic fields can drastically change predictions of evolutionary models of massive stars via mass-loss quenching, magnetic braking, and efficient angular…”
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First results from the LIFE project: discovery of two magnetic hot evolved stars
Published in Monthly notices of the Royal Astronomical Society (01-04-2018)“…Abstract We present the initial results of the Large Impact of magnetic Fields on the Evolution of hot stars (LIFE) project. The focus of this project is the…”
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Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: evolution to the end of core helium burning
Published in Monthly notices of the Royal Astronomical Society (11-03-2015)“…Massive stars are key sources of radiative, kinetic and chemical feedback in the Universe. Grids of massive star models computed by different groups each using…”
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Bayesian sampling with BeAtlas, a grid of synthetic Be star spectra I. Recovering the fundamental parameters of α Eri and β CMi
Published in Monthly notices of the Royal Astronomical Society (29-09-2023)“…ABSTRACT Classical B emission (Be) stars are fast rotating, near-main-sequence B-type stars. The rotation and the presence of circumstellar discs profoundly…”
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Period–luminosity relations of fast-rotating B-type stars in the young open cluster NGC 3766
Published in Monthly notices of the Royal Astronomical Society (01-06-2017)“…Abstract We study the pulsational properties of rapidly rotating main-sequence B-type stars using linear non-adiabatic analysis of non-radial low-frequency…”
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