activity
20182025
most citedOn the sensitivity of gravito-inertial modes to differential rotation in intermediate-mass main-sequence stars

129 citations · 134 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2025

Tides in Massive Binaries: Numerical Solutions and Semi-Analytical Comparisons

Meng Sun, Hongbo Xia, Seth Gossage +5

We present a systematic comparison between the tidal secular evolution timescales predicted by the direct numerical method and those given by the commonly used semi-analytic prescr…

astro-ph.SR2025

Numerical Non-Adiabatic Tidal Calculations with GYRE-tides: The WASP-12 Test Case

Meng Sun, Richard H. D. Townsend, Hongbo Xia +1

We revisit the tidal evolution of the WASP-12 system using direct numerical calculations with the GYRE-tides code. WASP-12b is a hot Jupiter on a 1.1-day orbit around a slightly ev…

astro-ph.SR2024

The impact of radiative levitation on mode excitation of main-sequence B-type pulsators

R. Rehm, J. S. G. Mombarg, C. Aerts +3

Numerical computations of stellar oscillations for models representative of B-type stars predict fewer modes to be excited than observations reveal from modern space-based photomet…

astro-ph.EP2024★ 4 cited

The coevolution of migrating planets and their pulsating stars through episodic resonance locking

Jared Bryan, Julien de Wit, Meng Sun +2

Hot Jupiters are expected to form far from their host star and move toward close-in, circular orbits via a smooth, monotonic decay due to mild and constant tidal dissipation. Yet,…

astro-ph.SR2023

Modelling time-dependent convective penetration in 1D stellar evolution

Cole Johnston, Mathias Michielsen, Evan H. Anders +7

1D stellar evolution calculations produce uncertain predictions for quantities like the age, core mass, core compactness, and nucleo-synthetic yields; a key source of uncertainty i…

astro-ph.SR2023

MESA-Web: A cloud resource for stellar evolution in astronomy curricula

Carl E. Fields, Richard H. D. Townsend, A. L. Dotter +2

We present MESA-Web, a cloud resource with an online interface to the Modules for Experiments in Stellar Astrophysics (MESA) software instrument. MESA-Web allows learners to evolve…

astro-ph.SR2023★ 1 cited

Stellar Cruise Control: Weakened Magnetic Braking Leads to Sustained Rapid Rotation of Old Stars

Nicholas Saunders, Jennifer L. van Saders, Alexander J. Lyttle +8

Despite a growing sample of precisely measured stellar rotation periods and ages, the strength of magnetic braking and the degree of departure from standard (Skumanich-like) spindo…

astro-ph.SR2018★ 129 cited

On the sensitivity of gravito-inertial modes to differential rotation in intermediate-mass main-sequence stars

T. Van Reeth, J. S. G. Mombarg, S. Mathis +9

Context. While rotation has a major impact on stellar structure and evolution, its effects are not well understood. Thanks to high- quality and long timebase photometric observatio…