activity
20002005
most citedDynamics of the circumstellar gas in the Herbig Ae stars BF Orionis, SV Cephei, WW Vulpeculae and XY Persei

32 citations · 47 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph200514 cited

Results from the Wide Angle Search for Planets Prototype (WASP0) II: Stellar Variability in the Pegasus Field

Stephen R. Kane, T. A. Lister, Andrew Collier Cameron +5

Recent wide-field photometric surveys which target a specific field for long durations are ideal for studying both long and short period stellar variability. Here we report on 75 v…

astro-ph20041 cited

Current Status of the SuperWASP Project

D. J. Christian, D. L. Pollacco, W. I. Clarkson +16

We present the current status of the SuperWASP project, a Wide Angle Search for Planets. SuperWASP consists of up to 8 individual cameras using ultra-wide field lenses backed by hi…

astro-ph2004

Inferring coronal structure using X-ray spectra: A Chandra study of AB Dor

G. A. J. Hussain, N. S. Brickhouse, A. K. Dupree +5

The Chandra X-ray observatory monitored the single cool star, AB Doradus, continuously for a period lasting 88ksec (1.98 Prot) in 2002 December with the LETG/HRC-S. The X-ray light…

astro-ph200432 cited

Dynamics of the circumstellar gas in the Herbig Ae stars BF Orionis, SV Cephei, WW Vulpeculae and XY Persei

A. Mora, C. Eiroa, A. Natta +22

We present high resolution (lambda / Delta_lambda = 49000) echelle spectra of the intermediate mass, pre-main sequence stars BF Ori, SV Cep, WW Wul and XY Per. The spectra cover th…

astro-ph2002

University of St.Andrews Open Cluster Survey for Hot Jupiters

R. A. Street, Keith Horne, A. Collier Cameron +7

We are using the Isaac Newton Telescope Wide Field Camera to survey open cluster fields for transiting hot Jupiter planets. Clusters were selected on the basis of visibility, richn…

astro-ph2000

tau Boo b: Not so bright, but just as heavy

Andrew Collier Cameron, Keith Horne, David James +2

We present new results derived from high-resolution optical spectra of the tau Boo system, secured in March-May 2000. The results do not show the same feature reported by Cameron e…