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20152026
most citedDust masses of young disks: constraining the initial solid reservoir for planet formation

204 citations · 547 across the 13 of their papers we have counts for

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astro-ph.SR2024★ 3 cited

Constraining the Stellar Masses and Origin of the Protostellar VLA 1623 System

Sarah I Sadavoy, Patrick Sheehan, John J. Tobin +6

We present ALMA Band 7 molecular line observations of the protostars within the VLA 1623 system. We map CO (3 - 2) in the circumbinary disk around VLA 1623A and the outflow…

astro-ph.SR2023★ 25 cited

FAUST VIII. The protostellar disk of VLA 1623-2417 W and its streamers imaged by ALMA

S. Mercimek, L. Podio, C. Codella +25

More than 50% of solar-mass stars form in multiple systems. It is therefore crucial to investigate how multiplicity affects the star and planet formation processes at the protostel…

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,…

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.SR2020

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…

astro-ph.SR2019

Determining the physical conditions of extremely young Class 0 circumbinary disk around VLA1623A

Cheng-Han Hsieh, Shih-Ping Lai, Pou-Ieng Cheong +3

We present detailed analysis of high-resolution C18O (2-1), SO (88-77), CO (3-2) and DCO+ (3-2) data obtained by the Atacama Large Millimeter/sub-millimeter Array (ALMA) towards a…