Search Results - "Meynet, Georges"
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Stellar winds and metal enrichment from fast-rotating Population III stars
Published in Monthly notices of the Royal Astronomical Society (01-10-2021)“…ABSTRACT Stellar winds from fast-rotating Population III (Pop III) stars have long been suspected to make important contributions to early metal enrichment, as…”
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Rotating massive stars: From first stars to gamma ray bursts
Published in Reviews of modern physics (17-01-2012)“…How does rotation change the evolution, end stages, and stellar winds as well as types of supernovae explosions? This question is not only of importance for…”
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Is GW190521 the merger of black holes from the first stellar generations?
Published in Monthly notices of the Royal Astronomical Society. Letters (01-03-2021)“…ABSTRACT GW190521 challenges our understanding of the late-stage evolution of massive stars and the effects of the pair instability in particular. We discuss…”
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The Time-averaged Mass-loss Rates of Red Supergiants as Revealed by Their Luminosity Functions in M31 and M33
Published in The Astrophysical journal (01-01-2023)“…Abstract Mass loss in red supergiants (RSGs) is generally recognized to be episodic, but mass-loss prescriptions fail to reflect this. Evolutionary models show…”
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THE EFFECTS OF STELLAR ROTATION. I. IMPACT ON THE IONIZING SPECTRA AND INTEGRATED PROPERTIES OF STELLAR POPULATIONS
Published in The Astrophysical journal (20-05-2012)“…We present a sample of synthetic massive stellar populations created using the Starburst99 evolutionary synthesis code and new sets of stellar evolutionary…”
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The Luminosity Function of Red Supergiants in M31
Published in The Astrophysical journal (20-01-2020)“…The mass-loss rates of red supergiant stars (RSGs) are poorly constrained by direct measurements, and yet the subsequent evolution of these stars depends…”
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Massive Black Holes Regulated by Luminous Blue Variable Mass Loss and Magnetic Fields
Published in The Astrophysical journal (01-09-2020)“…We investigate the effects of mass loss during the main-sequence (MS) and post-MS phases of massive star evolution on black hole (BH) birth masses. We compute…”
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THE EVOLUTION OF ROTATING STARS
Published in Annual review of astronomy and astrophysics (01-01-2000)“…In this article we first review the main physical effects to be considered in the building of evolutionary models of rotating stars on the Upper Main-Sequence…”
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Imprints of fast-rotating massive stars in the Galactic Bulge
Published in Nature (London) (28-04-2011)“…Spinstars lead the way NGC 6522, the oldest globular cluster in our Galaxy, probably witnessed the earliest phases of the chemical enrichment of the Universe,…”
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Spectacular Nucleosynthesis from Early Massive Stars
Published in Astrophysical journal. Letters (01-02-2024)“…Abstract Stars that formed with an initial mass of over 50 M ⊙ are very rare today, but they are thought to be more common in the early Universe. The fates of…”
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The Effective Temperatures and Physical Properties of Magellanic Cloud Red Supergiants: The Effects of Metallicity
Published in The Astrophysical journal (10-07-2006)“…We present moderate-resolution spectrophotometry of 36 red supergiants (RSGs) in the LMC and 37 RSGs in the SMC. Using the MARCS atmosphere models to fit this…”
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Yellow Supergiants in the Small Magellanic Cloud: Putting Current Evolutionary Theory to the Test
Published in The Astrophysical journal (20-08-2010)“…The yellow supergiant content of nearby galaxies provides a critical test of massive star evolutionary theory. While these stars are the brightest in a galaxy,…”
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13
HAYDN
Published in Experimental astronomy (01-06-2021)“…In the last decade, the Kepler and CoRoT space-photometry missions have demonstrated the potential of asteroseismology as a novel, versatile and powerful tool…”
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MAGNETIC BRAKING OF STELLAR CORES IN RED GIANTS AND SUPERGIANTS
Published in The Astrophysical journal (15-09-2014)Get full text
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How rotation affects masses and ages of classical Cepheids
Published in EPJ Web of Conferences (01-01-2017)“…Classical Cepheid variable stars are both sensitive astrophysical laboratories and accurate cosmic distance tracers. We have recently investigated how the…”
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Journal Article Conference Proceeding -
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Dynamical evolution of population III stellar systems and the resulting binary statistics
Published in Monthly notices of the Royal Astronomical Society (01-02-2021)“…ABSTRACT We use N-body simulations to study the dynamical evolution of population III (Pop III) stellar systems and the resulting binary statistics. We design…”
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Correction to: Dynamical evolution of population III stellar systems and the resulting binary statistics
Published in Monthly notices of the Royal Astronomical Society (13-04-2023)Get full text
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18
Evolution of blue supergiants and α Cygni variables: puzzling CNO surface abundances
Published in Monthly notices of the Royal Astronomical Society (01-08-2013)“…A massive star can enter the blue supergiant region either by evolving directly from the main sequence, or by evolving from a previous red supergiant stage…”
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Chemical Abundances in the Secondary Star in the Black Hole Binary A0620–00
Published in The Astrophysical journal (10-07-2004)“…Using a high-resolution spectrum of the secondary star in the black hole binary A0620-00, we have derived the stellar parameters and veiling caused by the…”
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The puzzle of the CNO abundances of α Cygni variables resolved by the Ledoux criterion
Published in Monthly notices of the Royal Astronomical Society. Letters (01-03-2014)“…Recent stellar evolution computations show that the blue supergiant (BSG) stars could come from two distinct populations: a first group arising from massive…”
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