activity
20032008
most citedThe stellar association around Gamma Velorum and its relationship with Vela OB2

261 citations · 609 across the 10 of their papers we have counts for

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Showing 2006 · astro-phShow all

6 papers · 2 filters

astro-ph200656 cited

The Keele-Exeter young cluster survey: I. Low mass pre-main sequence stars in NGC 2169

R. D Jeffries, J. M. Oliveira, Tim Naylor +2

We have used R_C I_C CCD photometry from the Isaac Newton telescope and intermediate resolution spectroscopy from the Gemini North telescope to identify and characterise low-mass (…

astro-ph20062 cited

Search for Giant Planets around White Dwarfs with HST, Spitzer, and VLT

S. Friedrich, H. Zinnecker, S. Correia +3

For the last three years we have performed a survey for young (<3 Gyrs) giant planets around nearby white dwarfs with HST, Spitzer, and VLT. Direct HST/NICMOS imaging of the seven…

astro-ph2006

Turbulence in the Molecular Interstellar Medium

M. H. Heyer, C. Brunt

The observational record of turbulence within the molecular gas phase of the interstellar medium is summarized. We briefly review the analysis methods used to recover the velocity…

astro-ph200640 cited

The Keck Aperture Masking Experiment: Near-Infrared Sizes of Dusty Wolf-Rayet Stars

J. D. Monnier, P. G. Tuthill, W. C. Danchi +2

We report the results of a high angular resolution near-infrared survey of dusty Wolf-Rayet stars using the Keck-1 Telescope, including new multi-wavelength images of the pinwheel…

astro-ph200677 cited

Kinematic structure in the young Sigma Orionis association

R. D. Jeffries, P. F. L. Maxted, J. M. Oliveira +1

We have used precise radial velocity measurements for a large number of candidate low-mass stars and brown dwarfs, to show that the young Sigma Ori ``cluster'' consists of two spat…

astro-ph200646 cited

Galaxies Under the Cosmic Microscope: Resolved Spectroscopy and New Constraints on the z=1 Tully-Fisher relation

M. Swinbank, R. Bower, G. P. Smith +5

We exploit the gravitational potential of massive cluster lenses to probe the emission line properties of six z=1 galaxies which appear as highly magnified luminous arcs. Using the…