activity
20162021
most citedSeismic evidence for near solid-body rotation in two Kepler subgiants and implications for angular momentum transport

69 citations · 210 across the 4 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2021

Stellar evolution models with entropy-calibrated mixing-length parameter: application to red giants

Federico Spada, Pierre Demarque, Friedrich Kupka

We present evolutionary models for solar-like stars with an improved treatment of convection that results in a more accurate estimate of the radius and effective temperature. This…

astro-ph.SR202069 cited

Seismic evidence for near solid-body rotation in two Kepler subgiants and implications for angular momentum transport

S. Deheuvels, J. Ballot, P. Eggenberger +3

Asteroseismic measurements of the internal rotation of subgiants and red giants all show the need for invoking a more efficient transport of angular momentum than theoretically pre…

astro-ph.SR202050 cited

Active red giants: close binaries versus single rapid rotators

Patrick Gaulme, Jason Jackiewicz, Federico Spada +7

The objective of this work is to determine what fraction of red-giant (RG) stars shows photometric rotational modulation, and understand its origin. One of the underlying questions…

astro-ph.SR2020

Common dynamo scaling in slowly rotating young and evolved stars

Jyri J. Lehtinen, Federico Spada, Maarit J. Käpylä +2

One interpretation of the activity and magnetism of late-type stars is that these both intensify with decreasing Rossby number up to a saturation level, suggesting that stellar dyn…

astro-ph.SR2019

Testing the entropy calibration of the radii of cool stars: models of alpha Centauri A and B

F. Spada, P. Demarque

We present models of alpha Centauri A and B implementing an entropy calibration of the mixing-length parameter alpha_MLT, recently developed and successfully applied to the Sun (Sp…

astro-ph.SR2019

On the competing effect of wind braking and interior coupling in the rotational evolution of solar-like stars

F. Spada, A. C. Lanzafame

Solar-like stars (M < 1.3 Msun) lose angular momentum through their magnetized winds. The resulting evolution of the surface rotation period, which can be directly measured photome…