@article{guerrero:insu-03674431, TITLE = {{What Sets the Magnetic Field Strength and Cycle Period in Solar-type Stars?}}, AUTHOR = {Guerrero, G. and Zaire, B. and Smolarkiewicz, P. K. and de Gouveia Dal Pino, E. M. and Kosovichev, A. G. and Mansour, N. N.}, URL = {https://insu.hal.science/insu-03674431}, JOURNAL = {{The Astrophysical Journal}}, PUBLISHER = {{American Astronomical Society}}, VOLUME = {880}, YEAR = {2019}, DOI = {10.3847/1538-4357/ab224a}, KEYWORDS = {dynamo ; stars: magnetic field ; stars: rotation ; stars: solar-type ; Astrophysics - Solar and Stellar Astrophysics}, HAL_ID = {insu-03674431}, HAL_VERSION = {v1}, }