most citedChemically peculiar stars on the pre-main sequence

2 citations · 2 across the 6 of their papers we have counts for

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astro-ph.SR2025

A Census of Chemically Peculiar Stars in Stellar Associations

Lukas Kueß, Ernst Paunzen

The pre-main-sequence evolution of the chemically peculiar (CP) stars on the upper main sequence is still a vast mystery and not well understood. Our analysis of young associations…

astro-ph.SR2025

The Status of the Astrophysical Parameters of Upper Main Sequence Stars

Lukas Kueß, Ernst Paunzen

Calibrating the ages, masses, and radii of stars on the upper main sequence depends heavily on accurate measurements of the effective temperature () and surface gra…

astro-ph.SR2025

Lightcurves of stars in the Chamaeleon I Association

K. Neumannová, L. Kueß, E. Paunzen +1

Star-forming regions are essential for studying very young stellar objects of various masses. They still contain a significant amount of dust and gas. We present a study of light c…

astro-ph.SR2025

Symbiotic stars in Galactic open clusters

Lukas Kueß, Ernst Paunzen

The age determination of symbiotic stars is essential to put further constraints on models explaining these binary systems. In the Galactic field, this is especially problematic be…

astro-ph.SR2024

Apparent non-variable stars from the Kepler mission

E. Paunzen, F. Binder, A. Cyniburk +12

The analysis of non-variable stars is generally neglected in the literature. However, such objects are needed for many calibration processes and for testing pulsational models. The…

astro-ph.SR2024★ 2 cited

Chemically peculiar stars on the pre-main sequence

L. Kueß, E. Paunzen, N. Faltová +12

Context. The chemically peculiar (CP) stars of the upper main sequence are defined by spectral peculiarities that indicate unusual elemental abundance patterns in the presence of d…