
prof. dr hab. Andrzej Pigulski
ul. M. Kopernika 11
andrzej.pigulski@uwr.edu.pl
tel. +48 71 337 80 65, +48 71 372 93 73, +48 71 372 93 74
Zainteresowania
- be
- astronomy astrophysics
- space photometry
- stars oscillations
- early type stars
- stars early type
- massive stars
- stars massive
- stars rotation
- stars pulsation
Dyscyplina naukowa
- astronomia
Najnowsze publikacje
- 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
- BRITE photometry of the massive post-RLOF system HD149 404
- Seismic modelling of early B-type pulsators observed by BRITE – I. θ Ophiuchi
- The chaotic wind of WR 40 as probed by BRITE
- TESS first look at evolved compact pulsators
- Spectrum of the secondary component and new orbital elements of the massive triple star δ Ori A
- β Cas: The first δ Scuti star with a dynamo magnetic field
- Let there be more variability in two γ Cas stars
- Stellar masses from granulation and oscillations of 23 bright red giants observed by BRITE-Constellation
- Towards a consistent model of the hot quadruple system HD 93206 = QZ Carinæ I. Observations and their initial analyses
- TESS light curves of γ Cas stars
- International observational campaign of the 2014 eclipse of EE Cephei
- Mode identification and seismic study of δ Scuti, the prototype of a class of pulsating stars
- Revisiting the pulsational characteristics of the exoplanet host star β Pictoris
- Photometry of β Lyrae in 2018 by the BRITE Satellites
- HIDES spectroscopy of bright detached eclipsing binaries from the Kepler field - III. Spectral analysis, updated parameters and new systems
- ϵ Lupi: measuring the heartbeat of a doubly magnetic massive binary with BRITE Constellation
- Tidally excited oscillations in MACHO 80.7443.1718: Changing amplitudes and frequencies, high-frequency tidally excited mode, and a decrease in the orbital period
- HST/STIS analysis of the first main sequence pulsar CU Virginis