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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 2022Show all

6 papers · 1 filter

astro-ph.SR2022★ 4 cited

Progress towards a 3D Monte Carlo radiative transfer code for outflow wind modelling

Jakub Fišák, Jiří Kubát, Brankica Kubátová +2

Context: Radiative transfer modelling of expanding stellar envelopes is an important task in their analysis. To account for inhomogeneities and deviations from spherical symmetry,…

astro-ph.SR2022★ 17 cited

Analysis of photometric and spectroscopic variability of red supergiant Betelgeuse

Daniel Jadlovsky, Jiri Krticka, Ernst Paunzen +1

Betelgeuse is a pulsating red supergiant whose brightness is semi periodically variable and in February 2020 reached a historical minimum, the Great Dimming. The aims of this study…

astro-ph.SR2022★ 9 cited

HD 60431, the CP2 star with the shortest rotational period -- Physical parameters and period analysis

Z. Mikulasek, E. Semenko, E. Paunzen +5

CP2 stars show periodic photometric, spectroscopic, and magnetic variations with the rotational period. They are generally slow rotators, with rotational periods exceeding half a d…

astro-ph.SR2022★ 5 cited

Discovery and origin of the radio emission from the multiple stellar system KQVel

P. Leto, L. M. Oskinova, C. S. Buemi +20

KQVel is a binary system composed of a slowly rotating magnetic Ap star with a companion of unknown nature. In this paper, we report the detection of its radio emission. We conduct…

astro-ph.HE2022★ 6 cited

X-ray irradiation of the stellar wind in HMXBs with B supergiants: Implications for ULXs

J. Krticka, J. Kubat, I. Krtickova

Wind-fed high-mass X-ray binaries are powered by accretion of the radiatively driven wind on the compact star. Accretion-generated X-rays alter the ionization state of the wind. Be…

astro-ph.SR2022★ 7 cited

Photometric signatures of corotating magnetospheres of hot stars governed by higher-order magnetic multipoles

J. Krticka, Z. Mikulasek, P. Kurfurst +1

The light curves of magnetic, chemically peculiar stars typically show periodic variability due to surface spots that in most cases can be modeled by low-order harmonic expansion.…