Search Publications

Absolute parameters and period variation in a semidetached eclipsing variable V2247 Cyg
DOI: 10.48550/arXiv.1809.00884 Bibcode: 2018CoSka..48..536B

Volkov, I. M.; Ikonnikova, N. P.; Burlak, M. A.

We aim to determine the absolute parameters of the components of a poorly studied Algol-type eclipsing binary V2247 Cyg. The data analysis is based on our numerous precise UBVRcIc photometric observations and low resolution spectra. The photometric solution reveals a semi-detached configuration with a less-massive component filling its Roche lobe.…

2018 Contributions of the Astronomical Observatory Skalnate Pleso
Gaia 6
The nature of light variations in magnetic hot stars
Bibcode: 2018CoSka..48..170K

Niemczura, E.; Huang, L.; Krtička, J. +6 more

Magnetic stars show several types of light variability which is modulated by the stellar rotation. In chemically peculiar stars, the redistribution of the flux in the surface regions with peculiar chemical composition leads to the light variability with a typical amplitude of the order of hundredths of magnitude. The most efficient processes that …

2018 Contributions of the Astronomical Observatory Skalnate Pleso
IUE 5
Multiple, short-lived "stellar prominences" on the O giant ξ Persei: a magnetic star?
DOI: 10.48550/arXiv.1711.02531 Bibcode: 2018CoSka..48..305S

Henrichs, H. F.; Sudnik, N.

We present strong evidence for a rotation period of 2.0406 d of the O giant ξ Persei, derived from the NIV λ1718 wind line in 12 yr of IUE data. We predict that ξ Per has a magnetic dipole field, with superposed variable magnetic prominences. Favorable dates for future magnetic measurements can be predicted. We also analysed time-resolv…

2018 Contributions of the Astronomical Observatory Skalnate Pleso
IUE 1
Rotational properties of magnetic chemically peculiar stars
Bibcode: 2018CoSka..48..194N

Paunzen, E.; Bernhard, K.; Hümmerich, S. +1 more

The magnetic chemically peculiar (mCP) stars of the upper main sequence exhibit strong and globally organized magnetic fields that are inclined to the rotational axis and facilitate the development of surface abundance inhomogeneities resulting in photometric and spectroscopic variability. Photometric time series data are much easier to obtain tha…

2018 Contributions of the Astronomical Observatory Skalnate Pleso
Gaia 0