activity
20032024
most citedWeak magnetic fields in Ap/Bp stars: Evidence for a dipole field lower limit and a tentative interpretation of the magnetic dichotomy

296 citations · 1k across the 32 of their papers we have counts for

collaborators

32 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.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.SR2024★ 3 cited

SiO maser polarization and magnetic field in evolved cool stars

L. Marinho, F. Herpin, H. Wiesemeyer +6

Both magnetic fields and photospheric/atmospheric dynamics can be involved in triggering the important mass loss observed in evolved cool stars. Previous works have revealed that t…

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.SR2023★ 5 cited

Surface magnetism in the pulsating RV Tauri star R Scuti

Stefan Georgiev, Agnès Lèbre, Eric Josselin +3

We present the surface magnetic field conditions of the brightest pulsating RV Tauri star, R Sct. Our investigation is based on the longest spectropolarimetric survey ever performe…

astro-ph.SR2023★ 6 cited

The height of convective plumes in the red supergiant Cep

A. López Ariste, M. Wavasseur, Ph. Mathias +3

Aims. We seek to understand convection in red supergiants and the mechanisms that trigger the mass loss from cool evolved stars. Methods. Linear spectropolarimetry of the atomic li…