activity
20022014
most citedObservations of IC348: The Disk Population at 2-3 Million Years

462 citations · 949 across the 12 of their papers we have counts for

collaborators

12 papers

astro-ph.GA2014★ 9 cited

Photoionising feedback and the star formation rates in galaxies

J. M. MacLachlan, I. A. Bonnell, K. Wood +1

Aims. We investigate the effects of ionising photons on accretion and stellar mass growth in a young star forming region, using a Monte Carlo radiation transfer code coupled to a s…

astro-ph.EP2013★ 80 cited

Exoplanet Transit Variability: Bow Shocks and Winds Around HD 189733b

J Llama, A. A. Vidotto, M. Jardine +3

By analogy with the solar system, it is believed that stellar winds will form bow shocks around exoplanets. For hot Jupiters the bow shock will not form directly between the planet…

astro-ph.SR2012★ 1 cited

New brown dwarf disks in Upper Scorpius observed with WISE

P. Dawson, A. Scholz, T. P. Ray +5

We present a census of the disk population for UKIDSS selected brown dwarfs in the 5-10 Myr old Upper Scorpius OB association. For 116 objects originally identified in UKIDSS, the…

astro-ph.SR2011★ 40 cited

Shock formation around planets orbiting M-dwarf stars

A. A. Vidotto, J. Llama, M. Jardine +2

Bow shocks can be formed around planets due to their interaction with the coronal medium of the host stars. The net velocity of the particles impacting on the planet determines the…

astro-ph.CO2011★ 34 cited

The Stability of Low Surface Brightness Disks Based on Multi-Wavelength Modeling

John M. MacLachlan, Lynn D. Matthews, Kenneth Wood +1

To investigate the structure and composition of the dusty interstellar medium (ISM) of low surface brightness (LSB) disk galaxies, we have used multiwavelength photometry to constr…

astro-ph.SR2010★ 7 cited

A multiwavelength view of the protostellar binary IRAS04325+2402: a case for turbulent fragmentation

A. Scholz, K. Wood, D. Wilner +6

IRAS04325+2402 (herafter IRAS04325) is a complex protostellar system hosting two young stellar objects (AB and C in the following) at a separation of 1250AU. Here we present new de…