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20042024
most citedThe ALMA View of the OMC1 Explosion in Orion

96 citations · 615 across the 18 of their papers we have counts for

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Showing astro-ph.SRShow all

8 papers · 1 filter

astro-ph.SR202060 cited

Protoplanetary disk masses in NGC 2024: Evidence for two populations

Sierk E. van Terwisga, Ewine F. van Dishoeck, Rita K. Mann +8

Protoplanetary disks in dense, massive star-forming regions are strongly affected by their environment. How this environmental impact changes over time is an important constraint o…

astro-ph.SR201936 cited

High Precision Dynamical Masses of Pre-Main Sequence Stars with ALMA and Gaia

Patrick D. Sheehan, Ya-Lin Wu, Josh A. Eisner +1

The Keplerian rotation in protoplanetary disks can be used to robustly measure stellar masses at very high precision if the source distance is known. We present Atacama Large Milli…

astro-ph.SR2018

The Eccentric Cavity, Triple Rings, Two-Armed Spirals, and Double Clumps of the MWC 758 Disk

Ruobing Dong, Sheng-yuan Liu, Josh Eisner +15

Spatially resolved structures in protoplanetary disks hint at unseen planets. Previous imaging observations of the transitional disk around MWC 758 revealed an inner cavity, a ring…

astro-ph.SR2018

Protoplanetary Disk Properties in the Orion Nebula Cluster: Initial Results from Deep, High-Resolution ALMA Observations

J. A. Eisner, H. G. Arce, N. P. Ballering +13

We present ALMA 850 m continuum observations of the Orion Nebula Cluster that provide the highest angular resolution ( AU) and deepest sensitivity…

astro-ph.SR2018

Multiple Gaps in the Disk of the Class I Protostar GY 91

Patrick Sheehan, Josh Eisner

We present the highest spatial resolution ALMA observations to date of the Class I protostar GY 91 in the Ophiuchus L1688 molecular cloud complex. Our 870 m and 3 mm dust co…

astro-ph.SR201764 cited

Disk Masses for Embedded Class I Protostars in the Taurus Molecular Cloud

Patrick D. Sheehan, Josh A. Eisner

Class I protostars are thought to represent an early stage in the lifetime of protoplanetary disks, when they are still embedded in their natal envelope. Here we measure the disk m…