Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs-Reference-Cited by-同舟云学术

Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs

Published:2021-04-22 Issue:7 Volume:5 Page:707-714
ISSN:2397-3366
Container-title:Nature Astronomy
language:en
Short-container-title:Nat Astron

Author:

Hall Oliver J.^ORCID,Davies Guy R.,van Saders Jennifer,Nielsen Martin B.,Lund Mikkel N.,Chaplin William J.^ORCID,García Rafael A.^ORCID,Amard Louis^ORCID,Breimann Angela A.,Khan Saniya,See Victor,Tayar Jamie^ORCID

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://www.nature.com/articles/s41550-021-01335-x.pdf

Reference77 articles.

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3. Leiner, E., Mathieu, R. D., Vanderburg, A., Gosnell, N. M. & Smith, J. C. Blue Lurkers: hidden blue stragglers on the M67 main sequence identified from their Kepler/K2 rotation periods. Astrophys. J. 881, 47 (2019).

4. Claytor, Z. R. et al. Chemical evolution in the Milky Way: rotation-based ages for APOGEE-Kepler cool dwarf stars. Astrophys. J. 888, 43 (2020).

5. Barnes, S. A., Weingrill, J., Fritzewski, D., Strassmeier, K. G. & Platais, I. Rotation periods for cool stars in the 4 Gyr old Open Cluster M67, the solar-stellar connection, and the applicability of gyrochronology to at least solar age. Astrophys. J. 823, 16 (2016).

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