Stellar activity analysis of Barnard's Star: very slow rotation and evidence for long-term activity cycle
Autor(es) y otros:
Fecha de publicación:
2019
Versión del editor:
Citación:
Monthly Notices Of The Royal Astronomical Society, 488(4), p. 5145-5161 (2019); doi:10.1093/mnras/stz1975
Descripción física:
p. 5145-5161
Patrocinado por:
This work has been financed by the Spanish Ministry of Science, Innovation and Universities (MICIU) through the grant AYA2017- 86389-P. BTP acknowledges Fundacio ́n La Caixa for the finan- cial support received in the form of a Ph.D. contract. JIGH acknowledges financial support from the Spanish MICIU under the 2013 Ramo ́n y Cajal program MICIU RYC-2013-14875. The IAA-CSIC and UCM teams acknowledge support by the Spanish Ministry of Economy and Competitiveness (MINECO) through grants AYA2016-79425-C3- 1-P,AYA2016-79425-C3-2-P,AYA2016-79425-C3-3-P,ESP2014- 54362P, and ESP2017-87143R. IR, JCM, MP, and EH acknowledge support from the Spanish MINECO and the Fondo Europeo de Desarrollo Regional (FEDER) through grant ESP2016-80435-C2- 1-R
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