activity
20132022
most citedVariability of newly identified B-type stars observed by Kepler

49 citations · 148 across the 10 of their papers we have counts for

collaborators

13 papers

astro-ph.SR2022

The eclipsing binary systems with Scuti component -- II. AB Cas

A. Miszuda, P. A. Kołaczek-Szymański, W. Szewczuk +1

We present a complex study of the eclipsing binary system, AB Cas. The analysis of the whole TESS light curve, corrected for the binary effects, reveals 112 significant frequency p…

astro-ph.SR202217 cited

Asteroseismology of the double-radial mode Scuti star BP Pegasi

Jadwiga Daszyńska-Daszkiewicz, P. Walczak, A. A. Pamyatnykh +1

Using the ASAS data, we determine the pulsational frequencies of the high-amplitude Sct star BP Pegasi. The analysis revealed only the two known, independent frequencies. On th…

astro-ph.SR202225 cited

Seismic modeling of a very young SPB star -- KIC8264293

Wojciech Szewczuk, Przemysław Walczak, Jadwiga Daszyńska-Daszkiewicz +1

KIC8264293 is a fast rotating B-type pulsator observed by Kepler satellite. Its photometric variability is mainly due to pulsations in high-order g modes. Besides, we detected a we…

astro-ph.SR202120 cited

The eclipsing binary systems with Scuti component. I. KIC 10661783

A. Miszuda, W. Szewczuk, J. Daszyńska-Daszkiewicz

We present a comprehensive study of the eclipsing binary system KIC 10661783. The analysis of the whole Kepler light curve, corrected for the binary effects, reveals a rich oscilla…

astro-ph.SR2021

Mode identification and seismic study of Scuti, the prototype of a class of pulsating stars

Jadwiga Daszynska-Daszkiewicz, A. A. Pamyatnykh, P. Walczak +3

We present a seismic study of Scuti based on a mode identification from multicoulor photometry. The dominant frequency can be associated only with a radial mode and the second…

astro-ph.SR202149 cited

Variability of newly identified B-type stars observed by Kepler

Wojciech Szewczuk, Przemysław Walczak, Jadwiga Daszyńska-Daszkiewicz

Recent re-determination of stellar atmospheric parameters for a sample of stars observed during the {\it Kepler} mission allowed to enlarge the number of {\it Kepler} B-type stars.…