activity
20002026
most cited3-D radiative transfer in clumped hot star winds I. Influence of clumping on the resonance line formation

79 citations · 807 across the 52 of their papers we have counts for

collaborators

52 papers

astro-ph.SR2026

Supernova interactions with aspherical circumstellar material I: calculations of light curves, AB magnitudes, spectra, and polarisation

Petr Kurfürst, Georgi Bless, Jakub Fišák +5

We present an upgraded detailed numerical calculations of supernova (SN) interactions with significantly aspherical circumstellar matter (CSM), primarily formed as a disc or bipola…

astro-ph.SR2024

Unveiling stellar aurorae: Simulating auroral emission lines in hot stars induced by high-energy irradiation

Michal Kajan, Jiří Krtička, Jiří Kubát

Auroral emission lines result from the interaction between magnetic field and stellar wind, offering valuable insights into physical properties and processes occurring within magne…

astro-ph.HE2022★ 6 cited

X-ray irradiation of the stellar wind in HMXBs with B supergiants: Implications for ULXs

J. Krticka, J. Kubat, I. Krtickova

Wind-fed high-mass X-ray binaries are powered by accretion of the radiatively driven wind on the compact star. Accretion-generated X-rays alter the ionization state of the wind. Be…

hep-ex2021★ 14 cited

Study of the decays into charmonia and three light hadrons

LHCb collaboration, R. Aaij, A. S. W. Abdelmotteleb +996

Using proton-proton collision data, corresponding to an integrated luminosity of collected with the LHCb detector, seven decay modes of the meson into a or…

hep-ex2021★ 7 cited

Searches for rare and decays into four muons

LHCb collaboration, R. Aaij, A. S. W. Abdelmotteleb +997

Searches for rare and decays into four muons are performed using proton-proton collision data recorded by the LHCb experiment, corresponding to an integrated luminosi…

astro-ph.SR2021★ 33 cited

New mass-loss rates of B supergiants from global wind models

Jiri Krticka, Jiri Kubat, Iva Krtickova

Massive stars lose a significant fraction of mass during their evolution. However, the corresponding mass-loss rates are rather uncertain. To improve this, we calculated global lin…