1 citations · 1 across the 3 of their papers we have counts for
3 papers
Simulations of dynamo action in slowly rotating M dwarfs: Dependence on dimensionless parameters
C. A. Ortiz-Rodríguez, P. J. Käpylä, F. H. Navarrete +4
The aim of this study is to explore the magnetic and flow properties of fully convective M dwarfs as a function of rotation period Prot and magnetic Reynolds ReM and Prandlt number…
Origin of magnetism in early-type stars
J. P. Hidalgo, P. J. Käpylä, C. A. Ortiz-Rodríguez +3
According to our understanding of stellar evolution, early-type stars have radiative envelopes and convective cores due to a steep temperature gradient produced by the CNO cycle. S…
Simulations of fully convective M dwarfs: dynamo action with varying magnetic Prandtl numbers
Carolina A. Ortiz-Rodríguez, Dominik R. G. Schleicher, Petri J. Käpylä +1
M dwarfs are low-mass main-sequence stars, the most numerous type of stars in the solar neighbourhood, which are known to have significant magnetic activity. The aim of this work i…