activity
20172022
most citedThe first view of Scuti and Doradus stars with the TESS mission

125 citations · 305 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2020

Oscillations of 2D ESTER models. I. The adiabatic case

D. R. Reese, G. M. Mirouh, F. Espinosa Lara +2

Recent numerical and theoretical considerations have shown that low-degree acoustic modes in rapidly rotating stars follow an asymptotic formula and recent observations of pulsatio…

astro-ph.SR2019125 cited

The first view of Scuti and Doradus stars with the TESS mission

V. Antoci, M. S. Cunha, D. M. Bowman +63

We present the first asteroseismic results for Scuti and Doradus stars observed in Sectors 1 and 2 of the TESS mission. We utilise the 2-min cadence TESS data for a sample…

astro-ph.SR201959 cited

Rotational modulation in TESS B stars

L. A. Balona, G. Handler, S. Chowdhury +6

Light curves and periodograms of 160 B stars observed by the TESS space mission and 29 main-sequence B stars from Kepler and K2 were used to classify the variability type. There ar…

astro-ph.SR201930 cited

Asteroseismology of massive stars with the TESS mission: the runaway Beta Cep pulsator PHL 346 = HN Aqr

Gerald Handler, Andrzej Pigulski, Jadwiga Daszyńska-Daszkiewicz +21

We report an analysis of the first known Beta Cep pulsator observed by the TESS mission, the runaway star PHL 346 = HN Aqr. The star, previously known as a singly-periodic pulsator…

astro-ph.SR201990 cited

Diverse Variability of O and B Stars Revealed from 2-minute Cadence Light Curves in Sectors 1 and 2 of the TESS Mission: Selection of an Asteroseismic Sample

May G. Pedersen, Sowgata Chowdhury, Cole Johnston +18

Uncertainties in stellar structure and evolution theory are largest for stars undergoing core convection on the main sequence. A powerful way to calibrate the free parameters used…

astro-ph.SR2018

Mode Classification in Fast-Rotating Stars using a Convolutional Neural Network: Model-Based Regular Patterns in Scuti Stars

Giovanni M. Mirouh, George C. Angelou, Daniel R. Reese +1

Oscillation modes in fast-rotating stars can be split into several subclasses, each with their own properties. To date, seismology of these stars cannot rely on regular pattern ana…