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19992024
most citedThe aromatic infrared bands as seen by ISO-SWS: probing the PAH model

180 citations · 1.4k across the 32 of their papers we have counts for

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Showing 2015Show all

5 papers · 1 filter

astro-ph.SR2015★ 13 cited

Magnetic Field Structures in Star Forming Regions: Mid-Infrared Imaging Polarimetry of K3-50

Peter Barnes, Dan Li, Charles Telesco +7

We report new imaging polarimetry observations of the Galactic compact HII region K3-50 using CanariCam at the Gran Telescopio Canarias. We use a standard polarimetric analysis tec…

astro-ph.SR2015★ 45 cited

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…

astro-ph.SR2015★ 109 cited

A compact concentration of large grains in the HD142527 protoplanetary dust trap

Simon Casassus, Chris Wright, Sebastian Marino +11

A pathway to the formation of planetesimals, and eventually giant planets, may occur in concentrations of dust grains trapped in pressure maxima. Dramatic crescent-shaped dust conc…

astro-ph.SR2015

Mid-infrared spectroscopy of SVS13: Silicates, quartz and SiC in a protoplanetary disc

Takuya Fujiyoshi, Christopher M. Wright, Toby J. T. Moore

We present -band (813 m) spectroscopic observations of the low-mass, embedded pre-main-sequence close binary system SVS13. Absorption features are clearly detected which a…

astro-ph.EP2015★ 52 cited

Compact dust concentration in the MWC 758 protoplanetary disk

S. Marino, S. Casassus, S. Perez +5

The formation of planetesimals requires that primordial dust grains grow from micron- to km-sized bodies. Dust traps caused by gas pressure maxima have been proposed as regions whe…