H. Bruntt

TL;DR: In this paper, the authors report observations of the star HD175726 that lasted for 27 days during the first short run of the CoRoT mission, which reveals a high activity signal and the power spectrum presents an excess due to solar-like oscillations with a low signal-to-noise ratio.

TL;DR: In this paper, the absolute dimensions and abundances for the solar-type detached eclipsing binary V636 Cen were determined based on uv-by light curves, uvby-beta standard photometry, radial velocity observations, and high-resolution spectra.

TL;DR: In this article, the authors report observations of the G0 subgiant eta Boo made in 1998, in Balmer-line equivalent width with the 2.5m Nordic Optical Telescope and in velocity with the 24-inch Lick CAT.

TL;DR: In this paper, the authors measured the masses, radii, effective temperatures and metallicities of three eclipsing binary stars with a red giant component that displays solar-like oscillations and found that the scaling relations without corrections to Δν systematically overestimate the masses of the three red giants by 11.7, 13.7 and 18.9 percent, respectively.

TL;DR: In this article, a short-period binary star system with total eclipses and multi-periodic delta Scuti pulsations was analyzed using the Kepler satellite photometry of KIC 10661783.