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19992008
most citedKinematic structure in the young Sigma Orionis association

77 citations · 279 across the 5 of their papers we have counts for

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astro-ph200843 cited

The low-mass Initial Mass Function in the young cluster NGC 6611

J. M. Oliveira, R. D. Jeffries, J. Th. van Loon

NGC 6611 is the massive young cluster (2-3 Myr) that ionises the Eagle Nebula. We present very deep photometric observations of the central region of NGC 6611 obtained with the Hub…

astro-ph200868 cited

A survey for low mass spectroscopic binary stars in the young clusters around sigma Orionis and lambda Orionis

P. F. L. Maxted, R. D. Jeffries, J. M. Oliveira +2

We have obtained multi-epoch, high-resolution spectroscopy of 218 candidate low-mass stars and brown dwarfs in the young clusters around sigma Ori and lambda Ori. We find that 196…

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-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-ph200635 cited

Circumstellar discs in the young sigma Orionis cluster

J. M. Oliveira, R. D. Jeffries, J. Th. van Loon +1

We present new K- and L'-band imaging observations for members of the young (3-5 Myr) sigma Orionis cluster, obtained with UIST at UKIRT. We determine (K-L') colour excesses with r…

astro-ph2005

Circumstellar discs around solar-mass stars in NGC 6611

J. M. Oliveira, R. D. Jeffries, J. Th. van Loon +2

We have performed IZJHKL' observations in NGC 6611, the young cluster that ionises the Eagle Nebula. We have discovered a rich pre-main sequence concentrated around the O-stars in…