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

530 citations · 12.4k across the 226 of their papers we have counts for

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astro-ph.HE2018★ 125 cited

Kinematic links and the co-evolution of MHD winds, jets, and inner disks from a high-resolution optical [OI] survey

Andrea Banzatti, Ilaria Pascucci, Suzan Edwards +3

We present a survey of optical [OI] emission at 6300 Å toward 65 TTauri stars at the spectral resolution of km/s. Past work identified a highly blueshifted velocity compone…

astro-ph.EP2018★ 72 cited

The Ring Structure in the MWC 480 Disk Revealed by ALMA

Yao Liu, Giovanni Dipierro, Enrico Ragusa +20

Gap-like structures in protoplanetary disks are likely related to planet formation processes. In this paper, we present and analyze high resolution (0.17*0.11 arcsec) 1.3 mm ALMA c…

astro-ph.EP2018

Disk Winds and the Evolution of Planet-Forming Disks

I. Pascucci, S. Andrews, C. Chandler +1

Disk winds are thought to play an important role in the evolution and dispersal of planet-forming disks. While high-resolution optical and infrared spectroscopy has identified seve…

astro-ph.SR2018★ 530 cited

Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region

Feng Long, Paola Pinilla, Gregory J. Herczeg +23

Rings are the most frequently revealed substructure in ALMA dust observations of protoplanetary disks, but their origin is still hotly debated. In this paper, we identify dust subs…

astro-ph.SR2018★ 121 cited

A New Look at T Tauri Star Forbidden Lines: MHD Driven Winds from the Inner Disk

Min Fang, Ilaria Pascucci, Suzan Edwards +6

Magnetohydrodynamic (MHD) and photoevaporative winds are thought to play an important role in the evolution and dispersal of planet-forming disks. We report the first high-resoluti…

astro-ph.SR2018★ 26 cited

An ALMA Survey of faint disks in the Chamaeleon I star-forming region: Why are some Class II disks so faint?

Feng Long, Gregory J. Herczeg, Ilaria Pascucci +6

ALMA surveys of nearby star-forming regions have shown that the dust mass in the disk is correlated with the stellar mass, but with a large scatter. This scatter could indicate eit…