activity
20052026
most citedThe Disk Substructures at High Angular Resolution Project (DSHARP): I. Motivation, Sample, Calibration, and Overview

1.1k citations · 14.1k across the 174 of their papers we have counts for

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Showing 2021Show all

7 papers · 1 filter

astro-ph.EP2021★ 124 cited

Planetesimal rings as the cause of the Solar System's planetary architecture

Andre Izidoro, Rajdeep Dasgupta, Sean N. Raymond +3

Astronomical observations reveal that protoplanetary disks around young stars commonly have ring- and gap-like structures in their dust distributions. These features are associated…

astro-ph.EP2021★ 253 cited

A Circumplanetary Disk Around PDS70c

Myriam Benisty, Jaehan Bae, Stefano Facchini +14

PDS70 is a unique system in which two protoplanets, PDS70b and c, have been discovered within the dust-depleted cavity of their disk, at 22 and 34au respectively, by direct i…

astro-ph.EP2021★ 53 cited

Limits on Millimeter Continuum Emission from Circumplanetary Material in the DSHARP Disks

Sean M. Andrews, William Elder, Shangjia Zhang +10

We present a detailed analysis for a subset of the high resolution (~35 mas, or 5 au) ALMA observations from the Disk Substructures at High Angular Resolution Project (DSHARP) to s…

astro-ph.EP2021★ 35 cited

Vortex-like kinematic signal, spirals, and beam smearing effect in the HD 142527 disk

Y. Boehler, F. Ménard, C. M. T. Robert +8

Vortices are one of the most promising mechanisms to locally concentrate millimeter dust grains and allow the formation of planetesimals through gravitational collapse. The outer d…

astro-ph.GA2021★ 23 cited

The Core Mass Function in the Orion Nebula Cluster Region: What Determines the Final Stellar Masses?

Hideaki Takemura, Fumitaka Nakamura, Shuo Kong +29

Applying dendrogram analysis to the CARMA-NRO CO (=1--0) data having an angular resolution of 8", we identified 692 dense cores in the Orion Nebula Cluster (ONC) r…

astro-ph.SR2021★ 39 cited

FAUST II. Discovery of a Secondary Outflow in IRAS 15398-3359: Variability in Outflow Direction during the Earliest Stage of Star Formation?

Yuki Okoda, Yoko Oya, Logan Francis +66

We have observed the very low-mass Class 0 protostar IRAS 15398-3359 at scales ranging from 50 au to 1800 au, as part of the ALMA Large Program FAUST. We uncover a linear feature,…