A detailed overview of the knowledge gaps in our understanding of the heliospheric
interaction with the largely unexplored Very Local Interstellar Medium (VLISM) are provided …

Context. The wind-driven halo is a feature that is observed in images that were delivered by
the latest generation of ground-based instruments that are equipped with an extreme …

The orbital eccentricities of directly imaged exoplanets and brown dwarf companions
provide clues about their formation and dynamical histories. We combine new high-contrast …

Aims. HD 206893 is a nearby debris disk star that hosts a previously identified brown dwarf
companion with an orbital separation of∼ 10 au. Long-term precise radial velocity (RV) …

Debris belts on the periphery of planetary systems, encompassing the region occupied by
planetary orbits, are massive analogues of the Solar system's Kuiper belt. They are detected …

The protoplanetary disks seen around Herbig Ae stars eventually dissipate leaving just a
tenuous debris disk, comprised of planetesimals and the dust derived from them, as well as …

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 …

Context. HR 8799 is a young planetary system composed of four planets and a double
debris belt. Being the first multi-planetary system discovered with the direct imaging …

Over the past three decades, we have witnessed one of the great revolutions in our
understanding of the cosmos—the dawn of the Exoplanet Era. Where once we knew of just …

Context. Young nearby stars are good candidates in the search for planets with both radial
velocity (RV) and direct imaging techniques. This, in turn, allows for the computation of the …