413 citations
- Friedrich Schiller University JenaDE31 papers
- Centre National de la Recherche ScientifiqueFR8 papers
- Helmholtz Institute JenaDE7 papers
- Fraunhofer Institute for Applied Optics and Precision EngineeringDE6 papers
- Max Planck Institute for the Science of LightDE5 papers
- GSI Helmholtz Centre for Heavy Ion ResearchDE4 papers
- Max Planck Institute for AstronomyDE4 papers
- Pennsylvania State UniversityUS4 papers
- University of CambridgeGB4 papers
- University of TrentoIT4 papers
- Astronomical ObservatoryRS3 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR3 papers
6 papers · 1 filter
First detection of HDO ice in a protoplanetary disk
Alexey Potapov, Piyush Kalambkar, Jeroen Bouwman +4
Protoplanetary disks are the birthplace of planets and planetary systems. Investigating the molecular inventory of disks is key to linking the chemical evolution of the interstella…
The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) III: The vertical structure of debris disks
Brianna Zawadzki, Anna Fehr, A. Meredith Hughes +37
Debris disks -- collisionally sustained belts of dust and sometimes gas around main sequence stars -- are remnants of planet formation processes and are found in systems ${\gtrsim}…
JWST/MIRI coronagraphic search for planets in systems with gapped exoKuiper belts and proper motion anomalies
R. Bendahan-West, S. Marino, A. L. Carter +17
Over the past decade, ALMA has uncovered a range of substructures within exoKuiper belts, pointing to a population of undetected planets. With JWST's sensitivity, we now have the o…
Evidence for SiO cloud nucleation in the rogue planet PSO J318
P. Mollière, H. Kühnle, E. C. Matthews +25
Silicate clouds are known to significantly impact the spectra of late L-type brown dwarfs, with observable absorption features at ~ 10 micron. JWST has reopened our window to the m…
Debris disc formation induced by planetary growth
Hiroshi Kobayashi, Torsten Loehne
Several hundred stars older than 10 million years have been observed to have infrared excesses. These observations are explained by dust grains formed by the collisional fragmentat…
Fuzzy Characterization of Near-Earth-Asteroids
Florian Freistetter
Due to close encounters with the inner planets, Near-Earth-Asteroids (NEAs) can have very chaotic orbits. Because of this chaoticity, a statistical treatment of the dynamical prope…