activity
20102024
most citedCombining BRITE and ground-based photometry for the Beta Cephei star Nu Eridani: impact on photometric pulsation mode identification and detection of several g modes

32 citations · 148 across the 16 of their papers we have counts for

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astro-ph.SR2024

Photometric sample of early B-type pulsators in eclipsing binaries observed with TESS

C. I. Eze, G. Handler

Asteroseismology coupled with eclipsing binary modelling shows a great potential in improving the efficiency of measurements or calibrations of the interior mixing profile in massi…

astro-ph.SR2024

Cephei pulsators in eclipsing binaries observed with TESS

Christian I. Eze, Gerald Handler

The combined strength of asteroseismology and empirical stellar basic parameter determinations for in-depth asteroseismic analysis of massive pulsators in eclipsing binaries shows…

astro-ph.SR2023

The GW Vir instability strip in the light of new observations of PG 1159 stars. Discovery of pulsations in the central star of Abell 72 and variability of RX J0122.9-7521

Paulina Sowicka, Gerald Handler, David Jones +9

We present the results of new time series photometric observations of 29 pre-white dwarf stars of PG 1159 spectral type, carried out in the years 2014-2022. For the majority of sta…

astro-ph.SR20234 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.SR202210 cited

Kepler and TESS Observations of PG 1159-035

Gabriela Oliveira da Rosa, S. O. Kepler, Alejandro H. Córsico +11

PG 1159-035 is the prototype of the DOV hot pre-white dwarf pulsators. It was observed during the Kepler satellite K2 mission for 69 days in 59 s cadence mode and by the TESS satel…

astro-ph.SR2022

Tidally Tilted Pulsators

Gerald Handler, Rahul Jayaraman, Donald W. Kurtz +2

The tidally tilted pulsators are a new type of oscillating star in close binary systems that have their pulsation axis in the orbital plane because of the tidal distortion caused b…