prof. Mgr. Jiří Krtička, Ph.D.
Professor, Department of Theoretical Physics and Astrophysics
office: pav. 06/03040
Kotlářská 267/2
611 37 Brno
| phone: | +420 549 49 5297 |
|---|---|
| e‑mail: |
Total number of publications: 216
2025
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Efficiency of viscous angular momentum transport in dissipating Be binaries
ASTROPHYSICS AND SPACE SCIENCE, year: 2025, volume: 370, edition: 10, DOI
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Horizontal flows in the atmospheres of chemically peculiar stars
Astronomy and Astrophysics, year: 2025, volume: 694, edition: February, DOI
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Low-metallicity massive single stars with rotation III. Source of ionization and C IV emission in I Zw 18
ASTRONOMY & ASTROPHYSICS, year: 2025, volume: 703, edition: November, DOI
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New line-driven wind mass-loss rates for OB stars with metallicities down to 0.01 Z⊙
ASTRONOMY & ASTROPHYSICS, year: 2025, volume: 702, edition: October, DOI
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Polarization of light from fast-rotating Wolf-Rayet stars: Monte Carlo simulations compared to the analytical formula
Astronomy and Astrophysics, year: 2025, volume: 698, edition: May, DOI
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Red giant–jet collisions in galactic nuclei I: 3D hydrodynamical model of a few stellar orbits
Monthly Notices of the Royal Astronomical Society, year: 2025, volume: 540, edition: 2, DOI
2024
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Current state and future developments in star-jet interactions models
Appearance and Dynamics of Accretion onto Black Holes, held 5-9 November, 2024 at Astronomical Institute, Czech Academy of Sciences, Prague, year: 2024
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HD 34736: an intensely magnetised double-lined spectroscopic binary with rapidly rotating chemically peculiar B-type components
Monthly Notices of the Royal Astronomical Society, year: 2024, volume: 535, edition: 3, DOI
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Hot subdwarf wind models with accurate abundances II. Helium-dominated merger products CD-46 8926 and CD-51 11879
Astronomy and Astrophysics, year: 2024, volume: 683, edition: March 2024, DOI
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New mass-loss rates of Magellanic Cloud B supergiants from global wind models
Astronomy and Astrophysics, year: 2024, volume: 681, edition: January 2024, DOI