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

49 citations · 210 across the 12 of their papers we have counts for

collaborators

16 papers

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.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.…

astro-ph.SR2020

Seismic analysis of the double-mode radial pulsator SX Phoenicis

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

We present the results of complex seismic analysis of the prototype star SX Phoenicis. This analysis consists of a simultaneous fitting of the two radial-mode frequencies, the corr…

astro-ph.SR20205 cited

Rotational modulation and single g-mode pulsation in the B9pSi star HD174356?

Z. Mikulasek, E. Paunzen, S. Huemmerich +19

Chemically peculiar (CP) stars of the upper main sequence are characterised by specific anomalies in the photospheric abundances of some chemical elements. The group of CP2 stars,…