activity
20132021
most citedWeakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs

94 citations · 463 across the 12 of their papers we have counts for

collaborators

15 papers

astro-ph.SR202126 cited

Magnetic and Rotational Evolution of CrB from Asteroseismology with TESS

Travis S. Metcalfe, Jennifer L. van Saders, Sarbani Basu +15

During the first half of main-sequence lifetimes, the evolution of rotation and magnetic activity in solar-type stars appears to be strongly coupled. Recent observations suggest th…

astro-ph.SR202194 cited

Weakened magnetic braking supported by asteroseismic rotation rates of Kepler dwarfs

Oliver J. Hall, Guy R. Davies, Jennifer van Saders +9

Studies using asteroseismic ages and rotation rates from star-spot rotation have indicated that standard age-rotation relations may break down roughly half-way through the main seq…

astro-ph.SR20215 cited

Field linkage and magnetic helicity density

K. Lund, M. Jardine, A. J. B. Russell +3

The helicity of a magnetic field is a fundamental property that is conserved in ideal MHD. It can be explored in the stellar context by mapping large-scale magnetic fields across s…

astro-ph.SR2021

Photometric variability as a proxy for magnetic activity and its dependence on metallicity

Victor See, Julia Roquette, Louis Amard +1

Understanding how the magnetic activity of low-mass stars depends on their fundamental parameters is an important goal of stellar astrophysics. Previous studies show that activity…

astro-ph.SR202040 cited

Alfvén-wave driven magnetic rotator winds from low-mass stars I: rotation dependences of magnetic braking and mass-loss rate

Munehito Shoda, Takeru K. Suzuki, Sean P. Matt +7

Observations of stellar rotation show that low-mass stars lose angular momentum during the main sequence. We simulate the winds of Sun-like stars with a range of rotation rates, co…

astro-ph.SR2020

How much do underestimated field strengths from Zeeman-Doppler imaging affect spin-down torque estimates?

Victor See, Lisa Lehmann, Sean P. Matt +1

Numerous attempts to estimate the rate at which low-mass stars lose angular momentum over their lifetimes exist in the literature. One approach is to use magnetic maps derived from…