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20062009
most citedProtoplanetary Disk Structures in Ophiuchus

704 citations · 1.2k across the 7 of their papers we have counts for

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astro-ph20085 cited

The eSMA: description and first results

Sandrine Bottinelli, Ken H. Young, Richard Chamberlin +15

The eSMA ("extended SMA") combines the SMA, JCMT and CSO into a single facility, providing enhanced sensitivity and spatial resolution owing to the increased collecting area at the…

astro-ph200818 cited

The Structure of the DoAr 25 Circumstellar Disk

Sean M. Andrews, A. M. Hughes, D. J. Wilner +1

We present high spatial resolution (< 0.3" = 40$ AU) Submillimeter Array observations of the 865 micron continuum emission from the circumstellar disk around the young star DoAr 25…

astro-ph200890 cited

A Resolved Molecular Gas Disk around the Nearby A Star 49 Ceti

A. M. Hughes, D. J. Wilner, I. Kamp +1

The A star 49 Ceti, at a distance of 61 pc, is unusual in retaining a substantial quantity of molecular gas while exhibiting dust properties similar to those of a debris disk. We p…

astro-ph2008166 cited

Gas and Dust Emission at the Outer Edge of Protoplanetary Disks

A. M. Hughes, D. J. Wilner, C. Qi +1

We investigate the apparent discrepancy between gas and dust outer radii derived from millimeter observations of protoplanetary disks. Using 230 and 345 GHz continuum and CO J=3-2…

astro-ph2007159 cited

An Inner Hole in the Disk around TW Hydrae Resolved in 7 Millimeter Dust Emission

A. M. Hughes, D. J. Wilner, N. Calvet +3

We present Very Large Array observations at 7 millimeters wavelength that resolve the dust emission structure in the disk around the young star TW Hydrae at the scale of the ~4 AU…

astro-ph2006100 cited

Investigating grain growth in disks around southern T Tauri stars at millimetre wavelengths

Dave Lommen, Chris M. Wright, Sarah T. Maddison +7

CONTEXT - Low-mass stars form with disks in which the coagulation of grains may eventually lead to the formation of planets. It is not known when and where grain growth occurs, as…