126 citations · 188 across the 5 of their papers we have counts for
6 papers
High-resolution survey for planetary companions to young stars in the Taurus Molecular Cloud
A. L. Wallace, J. Kammerer, M. J. Ireland +6
Direct imaging in the infrared at the diffraction limit of large telescopes is a unique probe of the properties of young planetary systems. We survey 55 single class I and class II…
VLA cm-wave survey of young stellar objects in the Oph A cluster: constraining extreme UV- and X-ray-driven disk photo-evaporation -- A pathfinder for Square Kilometre Array studies
A. Coutens, H. B. Liu, I. Jiménez-Serra +28
Observations of young stellar objects (YSOs) in centimeter bands can probe the continuum emission from growing dust grains, ionized winds, and magnetospheric activity, which are in…
Fomalhaut debris disk emission at 7 millimeters: constraints on the collisional models of planetesimals
L. Ricci, L. Testi, S. T. Maddison +1
We present new spatially resolved observations of the dust thermal emission at 7 mm from the Fomalhaut debris disk obtained with the Australia Telescope Compact Array. These observ…
Physical Properties of Giant Molecular Clouds in the Large Magellanic Cloud
A. Hughes, T. Wong, J. Ott +14
The Magellanic Mopra Assessment (MAGMA) is a high angular resolution CO mapping survey of giant molecular clouds (GMCs) in the Large and Small Magellanic Clouds using the Mopra Tel…
3D SPH simulations of grain growth in protoplanetary disks
Guillaume Laibe, Jean-François Gonzalez, Laure Fouchet +1
We present the first results of the treatment of grain growth in our 3D, two-fluid (gas+dust) SPH code describing protoplanetary disks. We implement a scheme able to reproduce the…
3D SPH simulations of grain growth in protoplanetary disks
Guillaume Laibe, Jean-François Gonzalez, Laure Fouchet +1
We present the first results of the treatment of grain growth in our 3D, two-fluid (gas+dust) SPH code describing protoplanetary disks. We implement a scheme able to reproduce the…