TY  - JOUR
AU  - Cortés Contreras, Miriam
AU  - Montes Gutiérrez, David
PY  - 2019
DO  - 10.1051/0004-6361/201935315
SN  - 1432-0746
UR  - https://hdl.handle.net/20.500.14352/13570
T2  - Astronomy & astrophysics
AB  - Context. M dwarfs are known to generate the strongest magnetic fields among main-sequence stars with convective envelopes, but we are still lacking a consistent picture of the link between the magnetic fields and underlying dynamo mechanisms,...
LA  - eng
PB  - EDP Sciences S A
KW  - Rotation
KW  - evolution
KW  - Zeeman
KW  - Mass
KW  - Saturation
KW  - Topologies
KW  - Stars
KW  - Lines
KW  - Solar
TI  - Magnetic fields in M dwarfs from the CARMENES survey
TY  - journal article
VL  - 626
ER  -