We present the results of new global 3D MHD simulations of early M-Dwarf stars, exploring the influence that a tachocline of shear has on their instantaneous and long-term magnetic activity.
BT - Astrophysics and Space Science Proceedings DA - 2020-12 DO - 10.1007/978-3-030-55336-4_40 N2 -We present the results of new global 3D MHD simulations of early M-Dwarf stars, exploring the influence that a tachocline of shear has on their instantaneous and long-term magnetic activity.
PB - Springer International Publishing PY - 2020 SE - 285 SN - 9783030553357/1570-6591, 1570-6605 SP - 285 EP - 287 T2 - Astrophysics and Space Science Proceedings TI - Exploring the Origins of Intense Magnetism in Early M-Dwarf Stars VL - 57 ER -