
ul. M. Kopernika 11
wojciech.szewczuk@uwr.edu.pl
tel. +48 71 337 80 91, +48 71 372 93 73, +48 71 372 93 74
Zainteresowania
- astronomy astrophysics
- opacity
- stars opacity
- stars oscillations
- stars rotation
- stars evolution
- stars early–type
- stars early type
- convection
- asteroseismology
Dyscyplina naukowa
- astronomia
Najnowsze publikacje
- A Need to Revise Stellar Opacities from Asteroseismology of δ Scuti Stars
- The eclipsing binary systems with δ Scuti component I. KIC 10661783
- Asteroseismology of the double-radial mode δ Scuti star BP Pegasi
- Seismic analysis of the double-mode radial pulsator SX Phoenicis
- Seismic modelling of a very young SPB star – KIC 8264293
- Mode identification and seismic study of δ Scuti, the prototype of a class of pulsating stars
- The eclipsing binary systems with δ Scuti component – II. AB Cas
- Variability of newly identified B-type stars observed by Kepler
- Asteroseismology of double-mode radial δ Scuti stars: AE Ursae Majoris and RV Arietis
- Asteroseismology of the fast-rotating high-amplitude δ Scuti star V2367 Cygni
- KIC 3240411 – the hottest known SPB star with the asymptotic g–mode period spacing
- Domains of pulsational instability of low-frequency modes in rotating upper main sequence stars
- Binary and seismic modelling of the Kepler system KIC 10661783 with the δ Scuti component
- Testing Stellar Opacities using Asteroseismology
- Evolutionary and Seismic Modeling of the δ Sct Pulsator in a Binary System AB Cassiopeia
- Deciphering the period spacing pattern in the oscillation spectrum of the SPB star KIC 7760680