activity
19982026
most citedThe stellar association around Gamma Velorum and its relationship with Vela OB2

261 citations · 7.8k across the 156 of their papers we have counts for

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Showing 2004Show all

6 papers · 1 filter

astro-ph2004★ 39 cited

Contamination and exclusion in the sigma Orionis young group

Ben Burningham, Tim Naylor, S. P. Littlefair +1

We present radial velocities for 38 low-mass candidate members of the sigma Orionis young group. We have measured their radial velocities by cross-correlation of high resolution (R…

astro-ph2004★ 126 cited

The Lithium Depletion Boundary in NGC 2547 as a test of pre-main-sequence evolutionary models

R. D. Jeffries, J. M. Oliveira

Intermediate resolution spectroscopy from the ESO Very Large Telescope is analysed for 63 photometrically selected low-mass (0.08-0.30 Msun) candidates of the open cluster NGC 2547…

astro-ph2004★ 28 cited

Pre-main-sequence Lithium Depletion

R. D. Jeffries

In this review I briefly discuss the theory of pre-main-sequence (PMS) Li depletion in low-mass (0.075<M<1.2 Msun) stars and highlight those uncertain parameters which lead to subs…

astro-ph2004

Membership, binarity and accretion among very low-mass stars and brown dwarfs of the Sigma Orionis cluster

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

Intermediate resolution (R=7000) spectroscopy is presented for 76 photometrically selected very low mass (0.04<M<0.3M_{sun}) candidate members of the Sigma Orionis cluster. More th…

astro-ph2004

The Li Overabundance of J37: Diffusion or Accretion?

J. F. Ashwell, R. D. Jeffries, B. Smalley +3

In September 2002 the discovery of a super Li-rich F-dwarf (J37) in NGC 6633, an iron poor analogue of the better studied Hyades and Praecepe open clusters, was announced. This uni…

astro-ph2004★ 55 cited

Low mass stars, brown dwarf candidates and the mass function of the young open cluster NGC 2547

R. D. Jeffries, Tim Naylor, C. R. Devey +1

We present a catalogue of RIZ photometry over an area of 0.855 square degrees, centred on NGC 2547. The survey is substantially complete to limits of R_c=21.5, I_c=19.5, Z=19.5. We…