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20072026
most citedGaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region

530 citations · 5.5k across the 90 of their papers we have counts for

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Showing 2020Show all

6 papers · 1 filter

astro-ph.SR2020★ 23 cited

Resolved molecular line observations reveal an inherited molecular layer in the young disk around TMC1A

Daniel Harsono, Matthijs van der Wiel, Per Bjerkeli +4

Physical processes that govern the star and planet formation sequence influence the chemical composition and evolution of protoplanetary disks. To understand the chemical compositi…

astro-ph.IM2020★ 49 cited

On the accuracy of the ALMA flux calibration in the time domain and across spectral windows

Logan Francis, Doug Johnstone, Gregory Herczeg +2

A diverse array of science goals require accurate flux calibration of observations with the Atacama Large Millimeter/Submillimeter array (ALMA), however, this goal remains challeng…

astro-ph.SR2020★ 3 cited

Temperature structures of embedded disks: young disks in Taurus are warm

Merel L. R. van 't Hoff, Daniel Harsono, John J. Tobin +6

The chemical composition of gas and ice in disks around young stars set the bulk composition of planets. In contrast to protoplanetary disks (Class II), young disks that are still…

astro-ph.EP2020★ 39 cited

Dual-Wavelength ALMA Observations of Dust Rings in Protoplanetary Disks

Feng Long, Paola Pinilla, Gregory J. Herczeg +13

We present new Atacama Large Millimeter/submillimeter Array (ALMA) observations for three protoplanetary disks in Taurus at 2.9\,mm and comparisons with previous 1.3\,mm data both…

astro-ph.EP2020★ 40 cited

Spirals inside the millimeter cavity of transition disk SR 21

G. A. Muro-Arena, C. Ginski, C. Dominik +22

Hydrodynamical simulations of planet-disk interactions suggest that planets may be responsible for a number of the sub-structures frequently observed in disks in both scattered lig…

astro-ph.SR2020★ 29 cited

Missing water in Class I protostellar disks

Daniel Harsono, Magnus Persson, Alyssa Ramos +10

Water is a key volatile that provides insights into the initial stages of planet formation. The low water abundances inferred from water observations toward low-mass protostellar o…