Near-IR and optical radial velocities of the active M dwarf star Gl 388 (AD Leo) with SPIRou at CFHT and SOPHIE at OHP A 2.23 day rotation period and no evidence for a corotating planet (2023)
Attributed to:
Astrophysics at the University of Exeter
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202245660
Publication URI: http://dx.doi.org/10.1051/0004-6361/202245660
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics