activity
19992025
most citedTheory and evidence of global Rossby waves in upper main-sequence stars: r-mode oscillations in many Kepler stars

130 citations · 990 across the 41 of their papers we have counts for

collaborators

41 papers

astro-ph.SR2025

Axisymmetric second order perturbations of rotating main sequence stars

Umin Lee

We calculate the second order perturbations driven by oscillation modes of rotating stars. Assuming that the typical amplitude of oscillation modes is small, we expand the pert…

astro-ph.SR2023★ 4 cited

HD 42477: coupled r modes, g modes and a p mode in an A0Vnne star

D. W. Kurtz, R. Jayaraman, P. Sowicka +4

Several studies have shown that a number of stars pulsating in p modes lie between the Cep and Sct instability strips in the Hertzsprung-Russell (HR) Diagram. At present, t…

astro-ph.SR2022★ 4 cited

Non-linear excitation of low frequency modes by overstable convective modes in rotating stars

Umin Lee

We discuss non-linear excitation and amplitude saturation of -modes, -modes and overstable convective (OsC) modes in early type main sequence stars, taking account of the eff…

astro-ph.SR2021★ 23 cited

Overstable Convective Modes in Rotating Early Type Stars

Umin Lee

We calculate overstable convective (OsC) modes of , , and main sequence stars. To compute non-adiabatic OsC modes in the core, we assume $(\nabla\cd…

astro-ph.SR2021★ 72 cited

Rotation of the convective core in Dor stars measured by dips in period spacings of g modes coupled with inertial modes

Hideyuki Saio, Masao Takata, Umin Lee +2

The relation of period spacing () versus period () of dipole prograde g modes is known to be useful to measure rotation rates in the g-mode cavity of rapidly rotating Do…

astro-ph.SR2020★ 38 cited

Transport of angular momentum by stochastically excited waves as an explanation for the outburst of the rapidly rotating Be star HD49330

C. Neiner, U. Lee, S. Mathis +3

HD49330 is a Be star that underwent an outburst during its five-month observation with the CoRoT satellite. An analysis of its light curve revealed several independent p and g puls…