204 citations · 1.3k across the 32 of their papers we have counts for
32 papers
Stochastic light variations in hot stars from wind instability: Finding photometric signatures and testing against the TESS data
Jiri Krticka, Achim Feldmeier
Line-driven wind instability is expected to cause small-scale wind inhomogeneities, X-ray emission, and wind line profile variability. The instability can already develop around th…
Light variations due to the line-driven wind instability and wind blanketing in O stars
J. Krticka, A. Feldmeier
A small fraction of the radiative flux emitted by hot stars is absorbed by their winds and redistributed towards longer wavelengths. This effect, which leads also to the heating of…
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…
Clumpy wind accretion in supergiant neutron star high mass X-ray binaries
E. Bozzo, L. Oskinova, A. Feldmeier +1
The accretion of the stellar wind material by a compact object represents the main mechanism powering the X-ray emission in classical supergiant high mass X-ray binaries and superg…
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…
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…