Předměty
Publikace
- Properties and nature of Be stars 31. The binary nature, light variability, physical elements, and emission-line changes of HD 813572019 | Matematicko-fyzikální fakulta
- Physical properties of beta Lyrae A and its opaque accretion disk2018 | Matematicko-fyzikální fakulta
- Improved model of the triple system V746 Cassiopeiae that has a bipolar magnetic field associated with the tertiary2018 | Matematicko-fyzikální fakulta
- xi Tauri: a unique laboratory to study the dynamic interaction in a compact hierarchical quadruple system2016 | Matematicko-fyzikální fakulta
- Properties and nature of Be stars 30. Reliable physical properties of a semi-detached B9.5e+G8III binary BR CMi = HD 61273 compared to those of other well studied semi-detached emission-line binaries2015 | Matematicko-fyzikální fakulta
- 2.5D magnetohydrodynamic models of circumstellar discs around FS CMa post-mergers - I. Non-stationary accretion stage2023 | Matematicko-fyzikální fakulta
- V1294 Aql = HD 184279: A bad boy among Be stars or an important clue to the Be phenomenon?2022 | Matematicko-fyzikální fakulta
- First detection of a magnetic field in low-luminosity B[e] stars New scenarios for the nature and evolutionary stages of FS CMa stars2022 | Matematicko-fyzikální fakulta
- Spectroscopy of the massive interacting binary UU Cassiopeiae2022 | Matematicko-fyzikální fakulta
- Quick Ultra-VIolet Kilonova surveyor (QUVIK)2022 | Matematicko-fyzikální fakulta
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