activity
20002020
most citedLarge-scale magnetic topologies of mid-M dwarfs

465 citations · 2.6k across the 35 of their papers we have counts for

collaborators

35 papers

astro-ph.IM2020★ 192 cited

The Pencil Code, a modular MPI code for partial differential equations and particles: multipurpose and multiuser-maintained

A. Brandenburg, A. Johansen, P. A. Bourdin +34

The Pencil Code is a highly modular physics-oriented simulation code that can be adapted to a wide range of applications. It is primarily designed to solve partial differential equ…

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.SR2013★ 201 cited

A Bcool magnetic snapshot survey of solar-type stars

S. C. Marsden, P. Petit, S. V. Jeffers +20

Stellar magnetic field measurements obtained from spectropolarimetry offer key data for activity and dynamo studies, and we present the results of a major high-resolution spectropo…

astro-ph.SR2012★ 99 cited

The radius and mass of the close solar twin 18 Sco derived from asteroseismology and interferometry

M. Bazot, M. J. Ireland, D. Huber +28

The growing interest in solar twins is motivated by the possibility of comparing them directly to the Sun. To carry on this kind of analysis, we need to know their physical charact…

astro-ph.SR2012★ 30 cited

Estimating the p-mode frequencies of the solar twin 18 Sco

M. Bazot, T. L. Campante, W. J. Chaplin +17

Solar twins have been a focus of attention for more than a decade, because their structure is extremely close to that of the Sun. Today, thanks to high-precision spectrometers, it…

astro-ph.SR2011

Nonlinear simulations of the convection-pulsation coupling

T. Gastine, B. Dintrans

In cold Cepheids close to the red edge of the classical instability strip, a strong coupling between the stellar pulsations and the surface convective motions occurs. This coupling…