
ul. M. Kopernika 11
jadwiga.daszynska-daszkiewicz@uwr.edu.pl
tel. +48 71 337 80 75, +48 71 372 93 73, +48 71 372 93 74
Zainteresowania
- astronomy astrophysics
- opacity
- stars oscillations
- stars opacity
- stars rotation
- early type stars
- stars early–type
- stars early type
- asteroseismology
- stellar pulsations
Dyscyplina naukowa
- astronomia
Najnowsze publikacje
- A Need to Revise Stellar Opacities from Asteroseismology of δ Scuti Stars
- Asteroseismology of massive stars with the TESS mission: The runaway β Cep pulsator PHL 346 = HN Aqr
- Diverse variability of O and B stars revealed from 2-minute cadence light curves in sectors 1 and 2 of the TESS mission: selection of an asteroseismic sample
- Age Determination of Galactic B-type Stars in Double-lined Eclipsing Binaries
- The eclipsing binary systems with δ Scuti component I. KIC 10661783
- KIC 5950759: a high-amplitude δ Sct star with amplitude and frequency modulation near the terminal age main sequence
- Seismic modelling of early B-type pulsators observed by BRITE – I. θ Ophiuchi
- 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
- The first view of δ Scuti and γ Doradus stars with the TESS mission
- 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
- Revising the evolutionary stage of HD 163899: the effects of convective overshooting and rotation
- 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
- Interpretation of the BRITE oscillation data of the hybrid pulsator ν Eridani: a call for the modification of stellar opacities