activity
20152023
most citedHST/STIS analysis of the first main sequence pulsar CU Vir

18 citations · 35 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2023★ 1 cited

EPIC 206197016: A very hot white dwarf orbited by a strongly irradiated red dwarf

J. Krticka, A. Kawka, Z. Mikulasek +7

Very precise satellite photometry has revealed a large number of variable stars whose variability is caused either by surface spots or by binarity. Detailed studies of such variabl…

astro-ph.SR2021★ 1 cited

Light variability of white dwarfs and subdwarfs due to surface abundance spots

J. Krticka, M. Prvak, I. Krtickova +2

Classical main-sequence chemically peculiar stars show light variability that originates in surface abundance spots. In the spots, the flux redistribution due to line (bound-bound)…

astro-ph.SR2020★ 6 cited

Understanding the rotational variability of K2 targets. HgMn star KIC 250152017 and blue horizontal branch star KIC 249660366

J. Krticka, A. Kawka, Z. Mikulasek +6

Ultraprecise space photometry enables us to reveal light variability even in stars that were previously deemed constant. A large group of such stars show variations that may be rot…

astro-ph.SR2020★ 9 cited

Distorted surfaces of magnetic helium-peculiar stars: An application to a Cen

J. Krticka, Z. Mikulasek, M. Prvak +3

Helium-peculiar magnetic chemically peculiar stars show variations of helium abundance across their surfaces. As a result of associated atmospheric scale height variations, the ste…

astro-ph.SR2019★ 18 cited

HST/STIS analysis of the first main sequence pulsar CU Vir

J. Krticka, Z. Mikulasek, G. W. Henry +9

CU Vir has been the first main sequence star that showed regular radio pulses that persist for decades, resembling the radio lighthouse of pulsars and interpreted as auroral radio…

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…