activity
20162024
most citedThe evolution of surface magnetic fields in young solar-type stars I: the first 250 Myr

189 citations · 378 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2024★ 2 cited

The origins of the magnetic field in tip-RGB, AGB and post-AGB stars

Renada Konstantinova-Antova, Stefan Georgiev, Agnès Lèbre +3

During the last decade and a half, the new generation spectropolarimeter Narval at Pic du Midi, France allowed the study of weak magnetic fields in cool giant stars that are fairly…

astro-ph.SR2023

A long-term study of the magnetic field and activity in the M giant RZ Ari

R. Konstantinova-Antova, S. Georgiev, A. Lèbre +12

We present a detailed long-term study of the single M6 III giant RZ~Ari to obtain direct and simultaneous measurements of the magnetic field, activity indicators, and radial veloci…

astro-ph.SR2017★ 146 cited

The evolution of surface magnetic fields in young solar-type stars II: The early main sequence (250-650 Myr)

C. P. Folsom, J. Bouvier, P. Petit +6

There is a large change in surface rotation rates of sun-like stars on the pre-main sequence and early main sequence. Since these stars have dynamo driven magnetic fields, this imp…

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.SR2016★ 189 cited

The evolution of surface magnetic fields in young solar-type stars I: the first 250 Myr

C. P. Folsom, P. Petit, J. Bouvier +8

The surface rotation rates of young solar-type stars vary rapidly with age from the end of the pre-main sequence through the early main sequence. Important changes in the dynamos o…