activity
20122018
most citedThermohaline instability and rotation-induced mixing. III - Grid of stellar models and asymptotic asteroseismic quantities from the pre-main sequence up to the AGB for low- and intermediate-mass stars at various metallicities

281 citations · 452 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2018★ 66 cited

The Gaia-ESO survey: impact of extra-mixing on C- and N-abundances of giant stars

N. Lagarde, C. Reylé, A. C. Robin +30

The GES survey using FLAMES at the VLT has obtained high-resolution UVES spectra for a large number of giant stars, allowing a determination of the abundances of the key chemical e…

astro-ph.SR2017★ 41 cited

The magnetic strip(s) in the advanced phases of stellar evolution - Theoretical convective turnover timescale and Rossby number for low- and intermediate-mass stars up to the AGB at various metallicities

C. Charbonnel, T. Decressin, N. Lagarde +7

Recent spectropolarimetric observations of otherwise ordinary G, K, and M giants revealed localized magnetic strips in the HRD coincident with the regions where the first dredge-up…

astro-ph.SR2017★ 64 cited

Population synthesis to constrain Galactic and Stellar Physics- I- Determining age and mass of thin-disc red-giant stars

N. Lagarde, A. C. Robin, C. Reylé +1

The cornerstone mission Gaia, together with complementary surveys, will revolutionize our understanding of the formation and history of our Galaxy, providing accurate stellar masse…

astro-ph.SR2015

Constraining angular momentum transport processes in stellar interiors with red-giant stars in the open cluster NGC6819

N. Lagarde, A. Miglio, P. Eggenberger +2

Clusters are excellent test benches for verification and improvement of stellar evolution theory. The recent detection of solar-like oscillations in G-K giants in the open cluster…

astro-ph.SR2012

An abundance study of the red giants in the seismology fields of the CoRoT satellite

T. Morel, A. Miglio, N. Lagarde +11

A precise characterisation of the red giants in the seismology fields of the CoRoT satellite is a prerequisite for further in-depth seismic modelling. The optical spectra obtained…

astro-ph.SR2012★ 281 cited

Thermohaline instability and rotation-induced mixing. III - Grid of stellar models and asymptotic asteroseismic quantities from the pre-main sequence up to the AGB for low- and intermediate-mass stars at various metallicities

N. Lagarde, T. Decressin, C. Charbonnel +3

The availability of asteroseismic constraints for a large sample of stars from the missions CoRoT and Kepler paves the way for various statistical studies of the seismic properties…