Rotation Periods of Candidate Single Late-M Dwarfs in TESS

Rotation Periods of Candidate Single Late-M Dwarfs in TESS

Recent studies suggest that the angular momentum evolution of late-M and brown dwarfs differs from the well-known spin-down evolution of hotter stars. Characterizing the distribution of rotation periods of these objects in the solar neighborhood can help elucidate this evolutionary pathway just abov...

Full description

Saved in:
Bibliographic Details
Main Authors: Samantha Lambier, Stanimir Metchev, Paulo Miles-Páez, Leslie Moranta, Dakota Wolfe, Joelene Hales, Jeffrey Martinovic
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astronomical Journal
Subjects:
M dwarf stars
Observational astronomy
Periodic variable stars
Stellar rotation
Online Access:https://doi.org/10.3847/1538-3881/adf195
Tags: Add Tag
No Tags, Be the first to tag this record!

Internet

https://doi.org/10.3847/1538-3881/adf195

Similar Items