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BU Canis Minoris -- the Most Compact Known Flat Doubly Eclipsing Quadruple System
Theodor Pribulla, Tamás Borkovits, Rahul Jayaraman +25
We have found that the 2+2 quadruple star system BU CMi is currently the most compact quadruple system known, with an extremely short outer period of only 121 days. The previous re…
The surface composition of six newly discovered chemically peculiar stars. Comparison to the HgMn stars Lep and Scl and the superficially normal B star Cap
Richard Monier, E. Niemczura, D. W. Kurtz +10
We report on a detailed abundance study of six bright, mostly southern, slowly rotating late B stars: HD~1279 (B8III), HD~99803 (B9V), HD~123445 (B9V), HD~147550 (B9V), HD~171961 (…
Bright Southern Variable Stars in the bRing Survey
Samuel N. Mellon, Eric E. Mamajek, Remko Stuik +9
Besides monitoring the bright star Pic during the near transit event for its giant exoplanet, the Pictoris b Ring (bRing) observatories at Siding Springs Observatory, Austr…
Revisiting the pulsational characteristics of the exoplanet host star Pictoris
K. Zwintz, D. R. Reese, C. Neiner +22
Exoplanet properties crucially depend on their host stars' parameters. In case the exoplanet host star shows pulsations, asteroseismology can be used for an improved description of…
Discovery of δ Scuti Pulsations in the Young Hybrid Debris Disk Star HD 156623
Samuel N. Mellon, Eric E. Mamajek, Konstanze Zwintz +11
The bRing robotic observatory network was built to search for circumplanetary material within the transiting Hill sphere of the exoplanet Pic b across its bright host star …
Studying bright variable stars with the Multi-site All-Sky CAmeRA (MASCARA)
O. Burggraaff, G. J. J. Talens, J. Spronck +6
The Multi-site All-Sky CAmeRA (MASCARA) aims to find the brightest transiting planet systems by monitoring the full sky at magnitudes , taking data every 6.4 seconds. The…