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Type II and anomalous Cepheids in the Kepler K2 mission
Monika I. Jurkovic, Emese Plachy, László Molnár +4
We present the results of the analysis of Type II and anomalous Cepheids using the data from the Kepler K2 mission. The precise light curves of these pulsating variable stars are t…
Orbital parallax of binary systems compared to GAIA DR3 and the parallax zero-point offset at bright magnitudes
Martin Groenewegen
(abridged)Multiple systems for which the astrometric and spectroscopic orbit are known offer the unique possibility of determining the distance to these systems directly without an…
The intrinsic reddening of the Magellanic Clouds as traced by background galaxies -- III. The Large Magellanic Cloud
Cameron P. M. Bell, Maria-Rosa L. Cioni, Angus H. Wright +15
We present a map of the total intrinsic reddening across ~90 deg of the Large Magellanic Cloud (LMC) derived using optical (ugriz) and near-infrared (IR; YJKs) spectral energ…
A WISE view on extreme AGB stars
Martin Groenewegen
(abridged) Variability is a key property of stars on the asymptotic giant branch (AGB). Their pulsation period is related to the luminosity and mass-loss rate (MLR) of the star. Lo…
The VMC Survey -- XLVIII. Classical Cepheids unveil the 3D geometry of the LMC
V. Ripepi, L. Chemin, R. Molinaro +12
We employed the {\it VISTA near-infrared survey of the Magellanic System} (VMC), to analyse the light curves of Cepheid stars (DCEPs) in…
A new and homogeneous metallicity scale for Galactic classical Cepheids II. The abundance of iron and alpha elements
R. da Silva, J. Crestani, G. Bono +18
Classical Cepheids are the most popular distance indicators and tracers of young stellar populations. The key advantage is that they are bright and they can be easily identified in…