TY  - JOUR
AU  - Cortés Contreras, Miriam
AU  - Montes Gutiérrez, David
PY  - 2019
DO  - 10.1051/0004-6361/201834788
SN  - 1432-0746
UR  - https://hdl.handle.net/20.500.14352/13304
T2  - Astronomy and astrophysics
AB  - Chromospheric modeling of observed differences in stellar activity lines is imperative to fully understand the upper atmospheres of late-type stars. We present one-dimensional parametrized chromosphere models computed with the atmosphere code PHOENIX...
LA  - eng
PB  - EDP Sciencies
KW  - Atmospheric models
KW  - Radiative-transfer
KW  - Flare stars
KW  - Lines
KW  - Components
TI  - The CARMENES search for exoplanets around M dwarfs Chromospheric modeling of M2-3V stars with PHOENIX
TY  - journal article
VL  - 623
ER  -