Modelling the rotation period distribution of M dwarfs in the Kepler field
Crossref DOI link: https://doi.org/10.1007/s10509-017-3225-6
Published Online: 2017-12-12
Published Print: 2018-01
Update policy: https://doi.org/10.1007/springer_crossmark_policy
Koen, Chris http://orcid.org/0000-0003-2291-2660
Funding for this research was provided by:
South African National Research Foundation
License valid from 2017-12-12