
ul. M. Kopernika 11
dawid.mozdzierski2@uwr.edu.pl
tel. +48 71 337 80 92, +48 71 372 93 73, +48 71 372 93 74
Zainteresowania
- astronomy astrophysics
- stars evolution
- early type stars
- stars early type
- massive stars
- stars massive
- stars rotation
- emission line stars
- stars emission line
- binaries spectroscopic
Dyscyplina naukowa
- astronomia
Najnowsze publikacje
- A survey for variable young stars with small telescopes: VI – Analysis of the outbursting Be stars NSW 284, gaia 19eyy, and VES 263
- A survey for variable young stars with small telescopes: II – mapping a protoplanetary disc with stable structures at 0.15 au
- An Absolute Calibration of the Near-infrared Period–Luminosity Relations of Type II Cepheids in the Milky Way and in the Large Magellanic Cloud
- Seismic modelling of a very young SPB star – KIC 8264293
- International observational campaign of the 2014 eclipse of EE Cephei
- Full orbital solution for the binary system in the northern Galactic disc microlensing event Gaia16aye
- Ensemble asteroseismology of pulsating B-type stars in NGC 6910
- Massive heartbeat stars from TESS
- BRITE observations of ν Centauri and γ Lupi, the first non-eclipsing members of the new class of nascent binaries
- A survey for variable young stars with small telescopes – IV. Rotation periods of YSOs in IC 5070
- A survey for variable young stars with small telescopes – VIII. Properties of 1687 Gaia selected members in 21 nearby clusters
- A survey for variable young stars with small telescopes – IX. Evolution of spot properties on YSOs in IC 5070
- Exploring extreme brightness variations in blue supergiant MACHO 80.7443.1718: Evidence for companion-driven enhanced mass loss
- Planet-Star Interactions with Precise Transit Timing. I. The Refined Orbital Decay Rate for WASP-12 b and Initial Constraints for HAT-P-23 b, KELT-1 b, KELT-16 b, WASP-33 b and WASP-103 b
- Solving the Mystery of Extreme Light Variability in the Massive Eccentric System MACHO 80.7443.1718
- Variability in NGC 6910, the open cluster rich in β Cephei-type stars