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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 2015Show all

5 papers · 1 filter

astro-ph.SR2015★ 27 cited

Modelling of variability of the chemically peculiar star phi Draconis

Milan Prvák, Jiří Liska, Jiří Krtička +2

Context: The presence of heavier chemical elements in stellar atmospheres influences the spectral energy distribution (SED) of stars. An uneven surface distribution of these elemen…

astro-ph.SR2015

Revisiting the Rigidly Rotating Magnetosphere model for Ori E - II. Magnetic Doppler imaging, arbitrary field RRM, and light variability

M. E. Oksala, O. Kochukhov, J. Krticka +6

The initial success of the Rigidly Rotating Magnetosphere (RRM) model application to the B2Vp star sigma OriE by Townsend, Owocki & Groote (2005) triggered a renewed era of observa…

astro-ph.SR2015★ 37 cited

X-ray irradiation of the winds in binaries with massive components

Jiri Krticka, Jiri Kubat, Iva Krtickova

Binaries with hot massive components are strong X-ray sources. Besides the intrinsic X-ray emission of individual binary members originating in their winds, X-ray emission stems fr…

astro-ph.SR2015★ 1 cited

Preliminary study of the moderately cool chemically peculiar star BS Circini

Zdenek Mikulasek, Jan Janik, Jiri Krticka +2

BS Cir is a representative of moderately cool magnetic chemically peculiar stars which displays very strong light variations in Stroemgren index c1 indicating large changes in the…

astro-ph.SR2015★ 30 cited

Visual and ultraviolet flux variability of the bright CP star Aur

J. Krticka, Z. Mikulasek, T. Luftinger +1

Chemically peculiar stars of the upper part of the main sequence show periodical variability in line intensities and continua, modulated by the stellar rotation, which is attribute…