activity
20132021
most citedThe first view of Scuti and Doradus stars with the TESS mission

125 citations · 478 across the 13 of their papers we have counts for

collaborators

17 papers

astro-ph.SR2021

PLATO Hare-and-Hounds exercise: Asteroseismic model fitting of main-sequence solar-like pulsators

M. S. Cunha, I. W. Roxburgh, V. Aguirre Børsen-Koch +19

Asteroseismology is a powerful tool to infer fundamental stellar properties. The use of these asteroseismic-inferred properties in a growing number of astrophysical contexts makes…

astro-ph.SR202064 cited

First evidence of inertial modes in Doradus stars: The core rotation revealed

R-M. Ouazzani, F. Lignières, M-A. Dupret +4

Gamma Doradus stars present an incredibly rich pulsation spectra, with gravito-inertial modes, in some cases supplemented with delta Scuti-like pressure modes and in numerous cases…

astro-ph.SR2020

The Aarhus red giants challenge II. Stellar oscillations in the red giant branch phase

J. Christensen-Dalsgaard, V. Silva Aguirre, S. Cassisi +23

Context. The large quantity of high-quality asteroseismic data that obtained from space-based photometric missions and the accuracy of the resulting frequencies motivate a careful…

astro-ph.SR2020

The prototype star Doradus observed by TESS

S. Christophe, V. Antoci, E. Brunsden +2

Doradus is the prototype star for the eponymous class of pulsating stars that consists of late A-early F main-sequence stars oscillating in low-frequency gravito-inertial modes…

astro-ph.SR2019

The Aarhus Red Giants Challenge I: Stellar structures in the red giant branch phase

V. Silva Aguirre, J. Christensen-Dalsgaard, S. Cassisi +23

(Abridged). We introduce the Aarhus Red Giants Challenge, a series of detailed comparisons between widely used stellar evolution and oscillation codes aiming at establishing the mi…

astro-ph.SR201971 cited

Gravity-mode period spacings and near-core rotation rates of 611 Doradus stars with \textit{Kepler}

Gang Li, Timothy Van Reeth, Timothy R. Bedding +4

We report our survey of \,Doradus stars from the 4-yr \textit{Kepler} mission. These stars pulsate mainly in g modes and r modes, showing period-spacing patterns in the amplitud…