Our understanding of planet formation has been rapidly evolving in recent years. The
classical planet formation theory, developed when the only known planetary system was our …

We describe a large-scale far-infrared line and continuum survey of protoplanetary disk
through to young debris disk systems carried out using the ACS instrument on the Herschel …

The protoplanetary system HD 169142 is one of the few cases where a potential candidate
protoplanet has recently been detected by direct imaging in the near-infrared. To study the …

Context. Herbig Ae/Be stars (HAeBes) have so far been studied based on relatively small
samples that are scattered throughout the sky. Their fundamental stellar and circumstellar …

We present L'-and J-band high-contrast observations of HD 169142, obtained with the Very
Large Telescope/NACO AGPM vector vortex coronagraph and the Gemini Planet Imager …

We present H-band Very Large Telescope/NACO polarized light images of the Herbig Ae/Be
star HD 169142 probing its protoplanetary disk as close as∼ 0 farcs 1 to the star. Our …

We observed a sample of 20 representative Herbig Ae/Be stars and 5 A-type debris discs
with PACS onboard Herschel, as part of the GAS in Protoplanetary Systems (GASPS) …

Context. The evolution of young massive protoplanetary disks toward planetary systems is
expected to correspond to structural changes in observational appearance, which includes …

HD 169142 is an excellent target for investigating signs of planet–disk interaction due to
previous evidence of gap structures. We perform J-band (∼ 1.2 μm) polarized intensity …

We present observations of the Herbig Ae star HD 169142 with the VLT/SPHERE
instruments InfraRed Dual-band Imager and Spectrograph (IRDIS)(K 1 K 2 and H 2 H 3 …