activity
20152024
most citedThe Kepler view of magnetic chemically peculiar stars

44 citations · 117 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.SR2024

New ACV variables discovered in the Zwicky Transient Facility survey

B. Bauer-Fasching, K. Bernhard, E. Brändli +8

The manifestation of surface spots on magnetic chemically peculiar (mCP) stars is most commonly explained by the atomic diffusion theory, which requires a calm stellar atmosphere a…

astro-ph.SR2023★ 19 cited

Photometric variability of the LAMOST sample of magnetic chemically peculiar stars as seen by TESS

J. Labadie-Bartz, S. Hümmerich, K. Bernhard +2

High-quality light curves from space missions have opened up a new window on the rotational and pulsational properties of magnetic chemically peculiar (mCP) stars and have fuelled…

astro-ph.GA2023★ 3 cited

High-velocity CP2 stars in the Galactic halo

Nikola Faltová, Michal Prišegen, Klaus Bernhard +2

Context. The second subclass of chemically peculiar stars, the CP2 stars, are early-type stars exhibiting anomalous abundances with variable line strengths possibly also accompanie…

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.SR2018★ 44 cited

The Kepler view of magnetic chemically peculiar stars

Stefan Hümmerich, Zdenek Mikulášek, Ernst Paunzen +6

Magnetic chemically peculiar (mCP) stars exhibit complex atmospheres that allow the investigation of such diverse phenomena as atomic diffusion, magnetic fields, and stellar rotati…

astro-ph.SR2018★ 25 cited

An investigation of the photometric variability of confirmed and candidate Galactic Be stars using ASAS-3 data

Klaus Bernhard, Sebastián Otero, Stefan Hümmerich +3

We present an investigation of a large sample of confirmed (N=233) and candidate (N=54) Galactic classical Be stars (mean V magnitude range of 6.4 to 12.6 mag), with the main aim o…

astro-ph.SR2017★ 18 cited

A Spectroscopic and Photometric Investigation of the Mercury-Manganese Star KIC 6128830

Stefan Hümmerich, Ewa Niemczura, Przemysław Walczak +4

The advent of space-based photometry provides the opportunity for the first precise characterizations of variability in Mercury-Manganese (HgMn/CP3) stars, which might advance our…

astro-ph.SR2016★ 7 cited

An Investigation of Four Chemically Peculiar Stars with Photometric Periods below 12 Hours

Stefan Hümmerich, Klaus Bernhard, Ernst Paunzen +3

We present an investigation of three chemically peculiar (CP) stars and one CP star candidate which exhibit photometric periods below 12 hours. New spectroscopic observations have…

astro-ph.SR2015

New Photometric Observations and the 2015 Eclipse of the Symbiotic Nova Candidate ASAS J174600-2321.3

Franz-Josef Hambsch, Stefan Hümmerich, Klaus Bernhard +1

The eclipsing binary system ASAS J174600-2321.3, which has shown a conspicuous brightening of ~4 magnitudes (V) in the past, was recently identified as a symbiotic nova candidate.…