activity
20122019
most citedBasic relations for the period variation models of variable stars

2 citations · 5 across the 7 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2019

Towards comprehension of the variability of the magnetic chemically peculiar star CU Virginis (HD 124224)

Zdeněk Mikulášek, Jiří Krtička, Andrzej Pigulski +2

The upper main sequence stars CU Virginis is the most enigmatic object among magnetic chemically peculiar (mCP) stars. It is an unusually fast rotator showing strictly periodic lig…

astro-ph.SR2019★ 1 cited

What is New with Landstreet Star HD 37776 (V901 Ori)?

Zdeněk Mikulášek, Jiří Krtička, Matthew E. Shultz +6

HD\,37776 (V901\,Ori, B2\,Vp), also known as Landstreet's Star, is possibly the most remarkable magnetic chemically peculiar (mCP) star known. Zeeman Doppler Imaging revealed this…

astro-ph.SR2019★ 1 cited

An overview of the properties of a sample of newly-identified magnetic chemically peculiar stars in the Kepler field

Zdeněk Mikulášek, Ernst Paunzen, Stefan Hümmerich +4

We present a comprehensive overview of the properties of a sample of 41 magnetic chemically peculiar stars that have been recently identified in the Kepler field by our team (Hümme…

astro-ph.SR2017

Monitoring of rotational period variations in magnetic chemically peculiar stars

Zdeněk Mikulášek

A majority part of magnetic chemically peculiar (mCP) stars of the upper main sequence exhibits strictly periodic light, magnetic, radio, and spectral variations that can be fully…

astro-ph.SR2016

Review of candidates of binary systems with an RR Lyrae component

Marek Skarka, Jiří Liška, Miloslav Zejda +1

We present an overview and current status of research on RR Lyrae stars in binary systems. In present days the number of binary candidates has steeply increased and suggested that…

astro-ph.SR2015★ 1 cited

The Concept of Few-Parameter Modelling of Eclipsing Binary and Exoplanet Transit Light Curves

Zdeněk Mikulášek, Miloslav Zejda, Theodor Pribulla +3

We present a new few-parameter phenomenological model of light curves of eclipsing binaries and stars with transiting planets that is able to fit the observed light curves with the…