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- Centre National de la Recherche ScientifiqueFR283 papers
- Joint Institute for Nuclear ResearchRU263 papers
- GSI Helmholtz Centre for Heavy Ion ResearchDE220 papers
- Polish Academy of SciencesPL180 papers
- National Centre for Nuclear ResearchPL173 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR168 papers
- University of WarsawPL166 papers
- Warsaw University of TechnologyPL166 papers
- National Research Nuclear University MEPhIRU163 papers
- Institut de Recherche sur les Lois Fondamentales de l'UniversFR155 papers
- The University of TokyoJP148 papers
- Institute of Nuclear Physics, Polish Academy of SciencesPL147 papers
16 papers · 2 filters
Orbital and physical parameters of eclipsing binaries from the All-Sky Automated Survey catalogue - X. Three high-contrast systems with secondaries detected with IR spectroscopy
K. G. Hełminiak, A. Tokovinin, E. Niemczura +13
We present results of the combined photometric and spectroscopic analysis of three detached eclipsing binaries, which secondary components are not visible or very hard to identify…
BRITE photometry of the massive post-RLOF system HD149404
G. Rauw, A. Pigulski, Y. Nazé +12
HD149404 is an evolved non-eclipsing O-star binary that has previously undergone a Roche lobe overflow interaction. Understanding some key properties of the system requires a deter…
LAMOST observations in the Kepler field. II. Database of the low-resolution spectra from the five-year regular survey
Weikai Zong, Jian-Ning Fu, Peter De Cat +19
The LAMOST-Kepler (LK-) project was initiated to use the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) to make spectroscopic follow-up observations for the tar…
A magnetic study of the Scuti variable HD 21190 and the close solar-type background star CPD -83 64B
S. P. Järvinen, S. Hubrig, R. -D. Scholz +3
HD 21190 is a known Scuti star showing Ap star characteristics and a variability period of 3.6 h discovered by the Hipparcos mission. Using Gaia DR1 data for an astrometric ana…
Short-term variability and mass loss in Be stars IV. Two groups of closely spaced, approximately equidistant frequencies in three decades of space photometry of Puppis (B7-8 IIIe)
D. Baade, A. Pigulski, Th. Rivinius +13
In early-type Be stars, groups of nonradial pulsation (NRP) modes with numerically related frequencies may be instrumental for the release of excess angular momentum through mass-e…
Variability survey in NGC 6910, the open cluster rich in Cephei-type stars
D. Moździerski, A. Pigulski, Z. Kołaczkowski +14
NGC 6910 is the northern hemisphere open cluster known to be rich in Cephei-type stars. Using four-season photometry obtained in Białków (Poland) and Xinglong (China) observato…