Debris disks are tenuous, dust-dominated disks commonly observed around stars over a
wide range of ages. Those around main sequence stars are analogous to the Solar System's …

A warm/hot dust component (at temperature 300 K) has been detected around 20% of A, F,
G, K stars. This component is called 'exozodiacal dust'as it presents similarities with the …

The cross-section of material in debris discs is thought to be dominated by the smallest
grains that can still stay in bound orbits despite the repelling action of stellar radiation …

We present stellar rotation rates derived from Transiting Exoplanet Survey Satellite (TESS)
light curves for stars in Upper Centaurus–Lupus (UCL;∼ 136 pc,∼ 16 Myr) and Lower …

Aims. We present new optical and near-infrared images of the debris disk around the F-type
star HD 114082 in the Scorpius-Centaurus OB association. We obtained direct imaging …

Extreme debris disks (EDDs) are rare systems with peculiarly large amounts of warm dust
that may stem from recent giant impacts between planetary embryos during the final phases …

Context. Debris disks are observed around 10 to 20% of FGK main-sequence stars as
infrared excess emission. They are important signposts for the presence of colliding …

While β Pic is known to host silicates in ring-like structures, whether the properties of these
silicate dust vary with stellocentric distance remains an open question. We re-analyze the β …

Context. Exoplanet properties crucially depend on the parameters of their host stars: more
accurate stellar parameters yield more accurate exoplanet characteristics. When the …

Abstract We have obtained Hubble Space Telescope STIS and NICMOS and Gemini/GPI
scattered-light images of the HD 191089 debris disk. We identify two spatial components: a …