4.3k citations
- European Southern ObservatoryCL197 papers
- National Radio Astronomy ObservatoryUS150 papers
- Centre National de la Recherche ScientifiqueFR140 papers
- National Astronomical Observatory of JapanJP134 papers
- Center for Astrophysics Harvard & SmithsonianUS101 papers
- Leiden UniversityNL98 papers
- Max Planck Institute for Radio AstronomyDE76 papers
- University of ChileCL71 papers
- University of CambridgeGB66 papers
- Max Planck Institute for AstronomyDE64 papers
- Institute of Astronomy and Astrophysics, Academia SinicaTW63 papers
- The Graduate University for Advanced Studies, SOKENDAIJP63 papers
5 papers · 2 filters
Millimeter Dust Emission and Planetary Dynamics in the HD 106906 System
Anna Fehr, A. Meredith Hughes, Rebekah I. Dawson +10
Debris disks are dusty, optically thin structures around main sequence stars. HD 106906AB is a short-period stellar binary, host to a wide separation planet, HD 106906b, and a debr…
Distributions of gas and small and large grains in the LkH disk trace a young planetary system
P. Pinilla, M. Benisty, N. T. Kurtovic +13
[abridged] We present new scattered light and millimeter observations of the protoplanetary disk around LkH, using SPHERE/VLT and ALMA, respectively. The scattered-light SP…
Multiwavelength Vertical Structure in the AU Mic Debris Disk: Characterizing the Collisional Cascade
David Vizgan, A. Meredith Hughes, Evan S. Carter +9
Debris disks are scaled-up analogs of the Kuiper Belt in which dust is generated by collisions between planetesimals. In the "collisional cascade" model of debris disks, dust lost…
Distribution of solids in the rings of the HD 163296 disk: a multiwavelength study
G. Guidi, A. Isella, L. Testi +15
In this paper we analyze new observations from ALMA and VLA, at a high angular resolution corresponding to 5 - 8 au, of the protoplanetary disk around HD 163296 to determine the du…
New Constraints on Protoplanetary Disk Gas Masses in Lupus
Dana E. Anderson, L. Ilsedore Cleeves, Geoffrey A. Blake +4
Gas mass is a fundamental quantity of protoplanetary disks that directly relates to their ability to form planets. Because we are unable to observe the bulk H content of disks…