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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)

First Author: Carmona A

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