Physically motivated heat-conduction treatment in simulations of solar-like stars: effects on dynamo transitions

Summary

This is a publication. If there is no link to the publication on this page, you can try the pre-formated search via the search engines listed on this page.

Authors: M. Viviani, M. J. Käpylä

Journal title: Astronomy & Astrophysics

Journal number: 645

Journal publisher: Springer Verlag

Published year: 2021

Published pages: A141

DOI identifier: 10.1051/0004-6361/202038603

ISSN: 0004-6361