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 …

Interplanetary dust particles and meteoroids mostly originate from comets and asteroids.
Understanding their distribution in the Solar system, their dynamical behavior and their …

We show that condensation is an efficient particle growth mechanism that leads to growth
beyond decimetre-sized pebbles close to an ice line in protoplanetary discs. As coagulation …

Context. Debris discs are a consequence of the planet formation process and constitute the
fingerprints of planetesimal systems. Their solar system counterparts are the asteroid and …

This paper presents a study of circumstellar debris around Sun-like stars using data from the
Herschel DEBRIS Key Programme. DEBRIS is an unbiased survey comprising the nearest∼ …

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 similar orbital distances and detection rates of debris disks and the prominent rings
observed in protoplanetary disks suggest a potential connection between these structures …

Abstract The Herschel DEBRIS (Disc Emission via a Bias-free Reconnaissance in the
Infrared/Submillimetre) survey brings us a unique perspective on the study of debris discs …

Context. Debris discs are a consequence of the planet formation process and constitute the
fingerprints of planetesimal systems. Their counterparts in the solar system are the asteroid …

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 …