activity
20162021
most citedNew and improved rotational periods of magnetic CP stars from ASAS-3, KELT and MASCARA data

35 citations · 40 across the 4 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

7 papers · 1 filter

astro-ph.SR2021

A case study of ACV variables discovered in the Zwicky Transient Facility survey

N. Faltová, K. Kallová, M. Prišegen +6

Magnetic chemically peculiar (mCP) stars exhibit complex atmospheres that allow the investigation of the interplay of atomic diffusion, magnetic fields, and stellar rotation. A non…

astro-ph.SR2020

High-Amplitude gamma Doradus Variables

Ernst Paunzen, Klaus Bernhard, Stefan Huemmerich +3

According to most literature sources, the amplitude of the pulsational variability observed in gamma Doradus stars does not exceed 0.1 mag in Johnson V. We have analyzed fifteen hi…

astro-ph.SR2020★ 5 cited

Rotational modulation and single g-mode pulsation in the B9pSi star HD174356?

Z. Mikulasek, E. Paunzen, S. Huemmerich +19

Chemically peculiar (CP) stars of the upper main sequence are characterised by specific anomalies in the photospheric abundances of some chemical elements. The group of CP2 stars,…

astro-ph.SR2020

A plethora of new, magnetic chemically peculiar stars from LAMOST DR4

Stefan Huemmerich, Ernst Paunzen, Klaus Bernhard

Magnetic chemically peculiar (mCP) stars are important to astrophysics because their complex atmospheres lend themselves perfectly to the investigation of the interplay between suc…

astro-ph.SR2018

TYC 3637-1152-1 - a High Amplitude delta Scuti star with peculiar pulsational properties

Ernst Paunzen, Klaus Bernhard, Moriz Frauenberger +16

In some delta Scuti stars, only one or two radial modes are excited (usually the fundamental mode and/or first overtone mode) and the observed peak-to-peak amplitudes exceed 0.3 ma…

astro-ph.SR2018

Orbital parameters and evolutionary status of the highly peculiar binary system HD 66051

E. Paunzen, M. Fedurco, K. G. Helminiak +8

The spectroscopic binary system HD 66051 (V414 Pup) consists of a highly peculiar CP3 (HgMn) star and an A-type component. It also shows out-of-eclipse variability that is due to c…