activity
20022017
most citedMagnetic Braking Formulation for Sun-Like Stars: Dependence on Dipole Field Strength and Rotation Rate

248 citations · 820 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.SR2017★ 31 cited

Frequency regularities of acoustic modes and multi-colour mode identification in rapidly rotating stars

D. R. Reese, F. Lignières, J. Ballot +4

Context: Mode identification has remained a major obstacle in the interpretation of pulsation spectra in rapidly rotating stars. Aims: We would like to test mode identification met…

astro-ph.SR2014★ 166 cited

Properties of 42 Solar-type Kepler Targets from the Asteroseismic Modeling Portal

T. S. Metcalfe, O. L. Creevey, G. Dogan +39

Recently the number of main-sequence and subgiant stars exhibiting solar-like oscillations that are resolved into individual mode frequencies has increased dramatically. While only…

astro-ph.SR2013

Oscillations and Surface Rotation of Red Giant Stars

Christina Hedges, Savita Mathur, Michael J. Thompson +1

More than 15000 red giants observed by Kepler for a duration of almost one year became public at the beginning of this year. We analysed a subsample of 416 stars to determine the g…

astro-ph.SR2012★ 48 cited

Mode visibilities in rapidly rotating stars

D. R. Reese, V. Prat, C. Barban +2

Context: Mode identification is a crucial step to comparing observed frequencies with theoretical ones, but has proven to be difficult in rapidly rotating stars. Aims: To further c…

astro-ph.SR2012★ 248 cited

Magnetic Braking Formulation for Sun-Like Stars: Dependence on Dipole Field Strength and Rotation Rate

Sean P. Matt, Keith B. MacGregor, Marc H. Pinsonneault +1

We use two-dimensional axisymmetric magnetohydrodynamic simulations to compute steady-state solutions for solar-like stellar winds from rotating stars with dipolar magnetic fields.…

astro-ph.SR2011★ 18 cited

Reflection and Ducting of Gravity Waves Inside the Sun

K. B. MacGregor, T. M. Rogers

Internal gravity waves excited by overshoot at the bottom of the convection zone can be influenced by rotation and by the strong toroidal magnetic field that is likely to be presen…