activity
20042024
most citedMulti-resonance orbital model of high-frequency quasi-periodic oscillations: possible high-precision determination of black hole and neutron star spin

157 citations · 984 across the 37 of their papers we have counts for

collaborators

37 papers

astro-ph.HE2024★ 1 cited

Accretion tori around rotating neutron stars II: Oscillations and precessions

Monika Matuszková, Gabriel Török, Kateřina Klimovičová +7

The four characteristic oscillation frequencies of accretion flows are, in addition to the Keplerian orbital frequency, often discussed in the context of the time variability of th…

astro-ph.HE2024★ 2 cited

Timing of accreting neutron stars with future X-ray instruments: towards new constraints on dense matter equation of state

V. Karas, K. Klimovicova, D. Lancova +7

The Enhanced X-ray Timing and Polarimetry (eXTP) mission is a space mission to be launched in the late 2020s that is currently in development led by China in international collabor…

astro-ph.HE2023★ 1 cited

Oscillations of Fluid Tori around Neutron Stars

Eva Šrámková, Monika Matuszková, Kateřina Klimovičová +7

We examine the influence of quadrupole moment of a slowly rotating neutron star (NS) on the oscillations of a fluid accretion disk (torus) orbiting a compact object the spacetime a…

astro-ph.HE2022★ 6 cited

Spectra of Puffy Accretion Discs: the kynbb Fit

Debora Lančová, Anastasiya Yilmaz, Maciek Wielgus +3

Puffy disc is a numerical model, expected to capture the properties of the accretion flow in X-ray black hole binaries in the luminous, mildly sub-Eddington state. We fit the kerrb…

astro-ph.HE2022★ 9 cited

Simple analytic formula relating the mass and spin of accreting compact objects to their rapid X-ray variability

Gabriel Török, Andrea Kotrlová, Monika Matuszková +4

Following the previous research on epicyclic oscillations of accretion disks around black holes (BHs) and neutron stars (NSs), a new model of high-frequency quasi-periodic oscillat…

astro-ph.HE2019★ 62 cited

Puffy accretion disks: sub-Eddington, optically thick, and stable

Debora Lančová, David Abarca, Włodek Kluźniak +6

We report on a new class of solutions of black hole accretion disks that we have found through three-dimensional, global, radiative magnetohydrodynamic simulations in general relat…