activity
19982023
most citedKepler Asteroseismology Program: Introduction and First Results

480 citations · 4.3k across the 108 of their papers we have counts for

collaborators

109 papers

astro-ph.SR2023

A calibration point for stellar evolution from massive star asteroseismology

Siemen Burssens, Dominic M. Bowman, Mathias Michielsen +10

Massive stars are progenitors of supernovae, neutron stars and black holes. During the hydrogen-core burning phase their convective cores are the prime drivers of their evolution,…

astro-ph.SR2023★ 17 cited

Internal Gravity Waves in Massive Stars II: Frequency Analysis Across Stellar Mass

R. P. Ratnasingam, T. M. Rogers, S. Chowdhury +4

Stars with masses above 1.6 solar masses generally possess convective cores and radiative envelopes, which allows the propagation of outward-travelling internal gravity waves. We h…

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.SR2023★ 6 cited

Comprehensive spectroscopic and photometric study of pulsating eclipsing binary star AI Hya

F. Kahraman Alicavus, T. Pawar, K. G. Hełminiak +9

The pulsating eclipsing binaries are remarkable systems that provide an opportunity to probe the stellar interior and to determine the fundamental stellar parameters precisely. Esp…

astro-ph.SR2022★ 10 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★ 18 cited

Tidally Tilted Pulsations in HD 265435, a subdwarf B Star with a Close White Dwarf Companion

Rahul Jayaraman, Gerald Handler, Saul Rappaport +4

Tidally tilted pulsators (TTPs) are an intriguing new class of oscillating stars in binary systems; in such stars, the pulsation axis coincides with the line of apsides, or semi-ma…