activity
19952023
most citedGrids of stellar models with rotation - I. Models from 0.8 to 120 Msun at solar metallicity (Z = 0.014)

1.7k citations · 9.5k across the 105 of their papers we have counts for

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Showing 2019Show all

6 papers · 1 filter

astro-ph.SR2019★ 54 cited

Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era

C. Charbonnel, N. Lagarde, G. Jasniewicz +7

Lithium is extensively known to be a good tracer of non-standard mixing processes occurring in stellar interiors. We present the results of a new large Lithium survey in red giant…

astro-ph.EP2019

The Search for Living Worlds and the Connection to Our Cosmic Origins

M. A. Barstow, S. Aigrain, J. Barstow +24

One of the most exciting scientific challenges is to detect Earth-like planets in the habitable zones of other stars in the galaxy and search for evidence of life. The ability to o…

astro-ph.GA2019★ 3 cited

Supermassive stars as the origin of the multiple populations in globular clusters

Mark Gieles, Corinne Charbonnel

Globular clusters (GCs) display anomalous light element abundances (HeCNONaMgAl), resembling the yields of hot-hydrogen burning, but there is no consensus yet on the origin of thes…

astro-ph.SR2019

Stellar Physics with High-Resolution UV Spectropolarimetry

Julien Morin, Jean-Claude Bouret, Coralie Neiner +26

Current burning issues in stellar physics, for both hot and cool stars, concern their magnetism. In hot stars, stable magnetic fields of fossil origin impact their stellar structur…

astro-ph.SR2019★ 25 cited

Evolution of rotation in rapidly rotating early-type stars during the main sequence with 2D models

D. Gagnier, M. Rieutord, C. Charbonnel +2

The understanding of the rotational evolution of early-type stars is deeply related to that of anisotropic mass and angular momentum loss. In this paper, we aim to clarify the rota…

astro-ph.SR2019★ 32 cited

Critical angular velocity and anisotropic mass loss of rotating stars with radiation-driven winds

D. Gagnier, M. Rieutord, C. Charbonnel +2

The understanding of the evolution of early-type stars is tightly related to that of the effects of rapid rotation. For massive stars, rapid rotation combines with their strong rad…