activity
20102026
most citedThe Disk Substructures at High Angular Resolution Project (DSHARP): I. Motivation, Sample, Calibration, and Overview

1.1k citations · 14.1k across the 130 of their papers we have counts for

collaborators
Showing 2016Show all

9 papers · 1 filter

astro-ph.EP2016★ 1 cited

Radial Drift of Dust in Protoplanetary Disks: The Evolution of Ice lines and Dead zones

Alex J. Cridland, Ralph E. Pudritz, Tilman Birnstiel

We have developed a new model for the astrochemical structure of a viscously evolving protoplanetary disk that couples an analytic description of the disk's temperature and density…

astro-ph.SR2016★ 24 cited

Testing dust trapping in the circumbinary disk around GG Tau A

P. Cazzoletti, L. Ricci, T. Birnstiel +1

The protoplanetary disk around the GGTau A binary system is so far one of the most studied young circumbinary disk. Observations of the dust continuum emission at sub-mm/mm wavelen…

astro-ph.EP2016★ 134 cited

Can dead zones create structures like a transition disk?

Paola Pinilla, Mario Flock, Maria de Juan Ovelar +1

[Abridged] Regions of low ionisation where the activity of the magneto-rotational instability is suppressed, the so-called dead zones, have been suggested to explain gaps and asymm…

astro-ph.EP2016★ 48 cited

Investigating dust trapping in transition disks with millimeter-wave polarization

A. Pohl, A. Kataoka, P. Pinilla +3

Spatially resolved polarized (sub-)mm emission has been observed for example in the protoplanetary disk around HL Tau. Magnetically aligned grains are commonly interpreted as the s…

astro-ph.SR2016★ 173 cited

Measuring Turbulence in TW Hya with ALMA: Methods and Limitations

Richard Teague, Stephane Guilloteau, Dmitry Semenov +7

We obtain high spatial and spectral resolution images of the CO J=2-1, CN N=2-1 and CS J=5-4 emission with ALMA in Cycle~2. The radial distribution of the turbulent broadening is d…

astro-ph.SR2016★ 302 cited

Dust Evolution and the Formation of Planetesimals

T. Birnstiel, M. Fang, A. Johansen

The solid content of circumstellar disks is inherited from the interstellar medium: dust particles of at most a micrometer in size. Protoplanetary disks are the environment where t…