266 citations · 908 across the 9 of their papers we have counts for
9 papers
Radio Monitoring of Protoplanetary Discs
C. Ubach, S. T. Maddison, C. M. Wright +3
Protoplanetary disc systems observed at radio wavelengths often show excess emission above that expected from a simple extrapolation of thermal dust emission observed at short mill…
Resolving structure of the disk around HD100546 at 7 mm with ATCA
Christopher Wright, Sarah Maddison, David Wilner +7
There is much evidence that planet formation is occurring in the disk around the Herbig Be star HD100546. To learn more about the processes occurring in this disk we conducted high…
Grain growth signatures in the protoplanetary discs of Chamaeleon and Lupus
Catarina Ubach, Sarah T. Maddison, Christopher M. Wright +3
We present ATCA results of a 3 and 7 mm continuum survey of 20 T Tauri stars in the Chamaeleon and Lupus star forming regions. This survey aims to identify protoplanetary discs wit…
Grain growth across protoplanetary discs: 10-micron silicate feature versus millimetre slope
Dave J. P. Lommen, Ewine F. van Dishoeck, Chris M. Wright +8
Young stars are formed within dusty discs. The grains in the disc are originally of the same size as interstellar dust. Models predict that these grains will grow in size through c…
PROSAC: A Submillimeter Array survey of low-mass protostars. II. The mass evolution of envelopes, disks, and stars from the Class 0 through I stages
Jes K. Jorgensen, Ewine F. van Dishoeck, Ruud Visser +5
The key question about early protostellar evolution is how matter is accreted from the large-scale molecular cloud, through the circumstellar disk onto the central star. A sample o…
Large grains in disks around young stars: ATCA observations of WW Cha, RU Lup, and CS Cha
Dave Lommen, Sarah Maddison, Chris Wright +3
Grains in disks around young stars grow from interstellar submicron sizes to planetesimals over the course of several Myr. Thermal emission of large grains or pebbles can be best o…