activity
20042017
most citedResolved Images of Large Cavities in Protoplanetary Transition Disks

650 citations · 3.8k across the 36 of their papers we have counts for

collaborators

36 papers

astro-ph.SR2017★ 70 cited

The Sizes and Depletions of the Dust and Gas Cavities in the Transitional Disk J160421.7-213028

Ruobing Dong, Nienke van der Marel, Jun Hashimoto +18

We report ALMA Cycle 2 observations of 230 GHz (1.3 mm) dust continuum emission, and CO, CO, and CO J = 2-1 line emission, from the Upper Scorpius transitional…

astro-ph.SR2016★ 9 cited

Velocity-resolved hot water emission detected toward HL Tau with the Submillimeter Array

Lars E. Kristensen, Joanna M. Brown, David Wilner +1

Using the Submillimeter Array (SMA) on Mauna Kea, the H2-16O 10_2,9-9_3,6 transition (E_up=1863K) at 321.2 GHz has been detected toward the embedded low-mass protostar HL Tau. The…

astro-ph.SR2014★ 11 cited

Herschel/PACS view of disks around low-mass stars and brown dwarfs in the TW Hya association

Yao Liu, Gregory J. Herczeg, Munan Gong +6

We conducted Herschel/PACS observations of five very low-mass stars or brown dwarfs located in the TW Hya association with the goal of characterizing the properties of disks in the…

astro-ph.SR2014

X-ray Emission from Young Stars in the TW Hya Association

Alexander Brown, Gregory J. Herczeg, Thomas R. Ayres +2

The 9 Myr old TW Hya Association (TWA) is the nearest group (typical distances of 50 pc) of pre-main-sequence (PMS) stars with ages less than 10 Myr and contains stars with b…

astro-ph.SR2013★ 34 cited

Probing the radial temperature structure of protoplanetary disks with Herschel/HIFI

D. Fedele, S. Bruderer, E. F. van Dishoeck +4

Herschel/HIFI spectroscopic observations of CO J=10-9, CO J=16-15 and [CII] towards HD 100546 are presented. The objective is to resolve the velocity profile of the lines to addres…

astro-ph.SR2013★ 2 cited

New X-ray Selected Pre-Main Sequence Members of the Serpens Molecular Cloud

Isa Oliveira, Margriet van der Laan, Joanna M. Brown

The study of young stars no longer surrounded by disks can greatly add to our understanding of how protoplanetary disks evolve and planets form. We have used VLT/FLAMES optical spe…