activity
20002022
most citedNew isolated planetary mass objects and the stellar and substellar mass function of the sigma Orionis cluster

137 citations · 861 across the 27 of their papers we have counts for

collaborators
Showing astro-phShow all

7 papers · 1 filter

astro-ph2008★ 37 cited

Chemical abundances of late-type pre-main sequence stars in the -Orionis cluster

J. I. González Hernández, J. A. Caballero, R. Rebolo +4

The young -Orionis cluster is an important location for understanding the formation and evolution of stars, brown dwarfs, and planetary-mass objects. Its metallicity, although b…

astro-ph2007★ 83 cited

The substellar mass function in sigma Orionis. II. Optical, near-infrared and IRAC/Spitzer photometry of young cluster brown dwarfs and planetary-mass objects

J. A. Caballero, V. J. S. Béjar, R. Rebolo +8

We investigate the mass function in the substellar domain down to a few Jupiter masses in the young sigma Orionis open cluster (3+/-2 Ma, d = 360^+70_-60 pc). We have performed a d…

astro-ph2005★ 36 cited

S Ori J053825.4-024241: A Classical T Tauri-like object at the substellar boundary

J. A. Caballero, E. L. Martín, M. R. Zapatero Osorio +4

We present a spectrophotometric analysis of S Ori J053825.4-024241, a candidate member close to the substellar boundary of the young (1-8 Myr), nearby (~360 pc) sigma Orionis star…

astro-ph2004★ 26 cited

The pre-main sequence spectroscopic binary UZ Tau East: improved orbital parameters and accretion phase dependence

Eduardo L. Martín, Antonio Magazzù, Xavier Delfosse +1

We present radial-velocity measurements obtained using high- and intermediate-resolution spectroscopic observations of the classical T Tauri star UZ Tau East obtained from 1994 to…

astro-ph2004★ 24 cited

An L0 dwarf companion in the brown dwarf desert, at 30 AU

T. Forveille, D. Ségransan, P. Delorme +8

We present the discovery of an L0 companion to the nearby M1.5 dwarf G 239-25, at a projected distance of 31 AU. It is the faintest companion discovered so far in our adaptive opti…

astro-ph2003

The sigma Orionis substellar population

David Barrado y Navascués, Víctor J. S. Béjar, Reinhard Mundt +4

VLT/FORS spectroscopy and 2MASS near-infrared photometry, together with previously known data, have been used to establish the membership and the properties of a sample of low-mass…