activity
20132026
most citedTime-dependent modeling of extended thin decretion disks of critically rotating stars

26 citations · 86 across the 12 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2026

What is the reason for the lack of cool evolved stars near the center of the Galaxy?

Petr Kurfürst, Michal Zajaček, Norbert Werner +2

The observed deficit of bright late-type giants in the central parsec of the Milky Way remains an open problem. We investigate whether repeated passages of red giants (RGs) through…

astro-ph.HE2026

Tidal disruption of a low-mass star in an active galactic nucleus as the origin of the PS16dtm outburst

Marzena Śniegowska, Bożena Czerny, Michal Zajaček +7

The event PS16dtm, which occured in the center of the Narrow Line Seyfert 1 (NLS1) galaxy SDSS J015804.75-005221.8 (z = 0.080440), is one of the few candidates for a tidal disrupti…

astro-ph.HE2026

Evolution of Quasi-Periodic Eruptions in the post-TDE Accretion Disk Perturbed by an Orbiting Star

Martin Mondek, Michal Zajaček, Henry Best +3

Quasi-periodic eruptions (QPEs) are a recently discovered class of highly variable X-ray bursts originating in galactic nuclei. These high-amplitude bursts exhibit periodicity rang…

astro-ph.SR2024★ 1 cited

Models of hot star decretion disks

Petr Kurfürst

Massive stars can during their evolution reach the phase of critical (or very rapid, near-critical) rotation when further increase in rotation rate is no longer kinematically allow…

astro-ph.HE2023★ 2 cited

Science with a small two-band UV-photometry mission III: Active Galactic Nuclei and nuclear transients

M. Zajaček, B. Czerny, V. K. Jaiswal +14

In this review (the third in the series focused on a small two-band UV-photometry mission), we assess possibilities for a small UV two-band photometry mission in studying accreting…

astro-ph.HE2023

Science with a small two-band UV-photometry mission I: Mission description and follow-up observations of stellar transients

N. Werner, J. Řípa, C. Thöne +33

This is the first in a collection of three papers introducing the science with an ultra-violet (UV) space telescope on an approximately 130~kg small satellite with a moderately fas…

astro-ph.SR2021★ 4 cited

Intrinsic polarization of Wolf-Rayet stars due to the rotational modulation of the stellar wind

S. Abdellaoui, J. Krtička, P. Kurfürst

Fast rotating Wolf-Rayet stars are expected to be progenitors of long duration gamma-ray bursts. However, the observational test of this model is problematic. Spectral lines of Wol…

astro-ph.GA2021★ 4 cited

A Survey of Novae in M83

A. W. Shafter, K. Hornoch, J. Benáček +14

The results of the first synoptic survey of novae in the barred spiral and starburst galaxy, M83 (NGC 5236), are presented. A total of 19 novae and one background supernova were di…

astro-ph.SR2017★ 18 cited

Two-dimensional modeling of density and thermal structure of dense circumstellar outflowing disks

Petr Kurfürst, Achim Feldmeier, Jiří Krtička

Context. Evolution of massive stars is affected by a significant loss of mass either via (nearly) spherically symmetric stellar winds or by aspherical mass-loss mechanisms, namely…

astro-ph.SR2016★ 18 cited

Torsional oscillations and observed rotational period variations in early-type stars

J. Krticka, Z. Mikulasek, G. W. Henry +2

Some chemically peculiar stars in the upper main sequence show rotational period variations of unknown origin. We propose these variations are a consequence of the propagation of i…

astro-ph.SR2014★ 13 cited

Magnetorotational instability in decretion disks of critically rotating stars and the outer structure of Be and Be/X-ray disks

Jiri Krticka, Petr Kurfurst, Iva Krtickova

Evolutionary models of fast-rotating stars show that the stellar rotational velocity may approach the critical speed. Critically rotating stars cannot spin up more, therefore they…

astro-ph.SR2014★ 26 cited

Time-dependent modeling of extended thin decretion disks of critically rotating stars

Petr Kurfürst, Achim Feldmeier, Jiří Krtička

During their evolution massive stars can reach the phase of critical rotation when a further increase in rotational speed is no longer possible. Direct centrifugal ejection from a…

astro-ph.SR2013

Models of extended decretion disks of critically rotating stars

Petr Kurfürst, Achim Feldmeier, Jiří Krtička

Massive stars may during their evolution reach the phase of critical rotation when the further increase in rotational speed is no longer possible. The ejection of matter in the equ…