13 citations · 30 across the 8 of their papers we have counts for
8 papers
Cluster characteristics of Galactic open clusters
K. Neumannová, J. Supíková, N. Faltová +4
Star clusters are perfectly suited for studying the formation, evolution, and dynamics of stars and their host galaxies. For this, we need to estimate total masses, radii and shape…
Open Superclusters II. Discovery of an Inactive Supercluster Including a New Star Cluster in the Solar Neighborhood
Juan Casado, Yasser Hendy, Nikola Faltova +1
The number of known star clusters, associations, and moving groups in the vicinity of the Sun has increased significantly due to the use of Gaia data. We investigated the existence…
An all-sky catalogue of stellar reddening values
E. Paunzen, M. Netopil, M. Prisegen +1
When observing astronomical objects, we must deal with extinction (i.e. the absorption and scattering of the emitted radiation by dust and gas between the source and the observer).…
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…
Uncovering new white dwarf - open cluster associations using Gaia DR3
M. Prišegen, N. Faltová
Context: Open clusters (OCs) provide homogeneous samples of white dwarfs (WDs) with known distances, extinctions, and total ages. The unprecedented astrometric precision of \textit…
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…
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…
White dwarf-open cluster associations based on Gaia DR2
M. Prišegen, M. Piecka, N. Faltová +2
Fundamental parameters and physical processes leading to the formation of white dwarfs (WDs) may be constrained and refined by discovering WDs in open clusters (OCs). Cluster membe…