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20002026
most citedMass loss in main-sequence B stars

115 citations · 1.7k across the 100 of their papers we have counts for

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Showing 2018Show all

5 papers · 1 filter

astro-ph.SR2018★ 26 cited

Wind inhibition by X-ray irradiation in HMXBs: the influence of clumping and the final X-ray luminosity

Jiri Krticka, Jiri Kubat, Iva Krtickova

In wind-powered X-ray binaries, the radiatively driven stellar wind from the primary may be inhibited by the X-ray irradiation. This creates the feedback that limits the X-ray lumi…

astro-ph.SR2018★ 5 cited

Hot-star wind models with magnetically split line blanketing

J. Krticka

Fraction of hot stars posses strong magnetic fields that channel their radiatively driven outflows. We study the influence of line splitting in the magnetic field (Zeeman effect) o…

astro-ph.SR2018★ 31 cited

Low-metallicity massive single stars with rotation. II. Predicting spectra and spectral classes of chemically-homogeneously evolving stars

B. Kubátová, D. Szécsi, A. A. C. Sander +7

Context. Metal-poor massive stars are supposed to be progenitors of certain supernovae, gamma-ray bursts and compact object mergers, potentially contributing to the early epochs of…

astro-ph.SR2018★ 30 cited

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…

astro-ph.SR2018★ 5 cited

The ultraviolet study of B[e] stars: evidence for pulsations, LBV-type variations, and processes in envelope

I. Krtickova, J. Krticka

Stars with B[e] phenomenon comprise a very diverse group of objects in a different evolutionary status. These objects show common spectral characteristics, including presence of Ba…