activity
20042012
most citedSpectroscopy of brown dwarf candidates in IC 348 and the determination of its substellar IMF down to planetary masses

76 citations · 658 across the 15 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2012★ 76 cited

Spectroscopy of brown dwarf candidates in IC 348 and the determination of its substellar IMF down to planetary masses

C. Alves de Oliveira, E. Moraux, J. Bouvier +4

Context. Brown dwarfs represent a sizable fraction of the stellar content of our Galaxy and populate the transition between the stellar and planetary mass regime. There is however…

astro-ph2008★ 12 cited

An IPHAS-based search for accreting very low-mass objects using VO tools

L. Valdivielso, E. L. Martin, H. Bouy +6

The main goal of this paper is to prove that accreting very low-mass stars and brown dwarfs can be identified in IPHAS, a Halpha emission survey of the northern Milky Way.Full expl…

astro-ph2008★ 42 cited

A deep look into the cores of young clusters I. sigma-Orionis

H. Bouy, N. Huelamo, E. L. Martin +9

Nearby young clusters are privileged places to study the star formation history. Over the last decade, the sigma-Orionis cluster has been a prime location for the study of young ve…

astro-ph2008★ 57 cited

Structural and compositional properties of brown dwarf disks: the case of 2MASS J04442713+2512164

H. Bouy, N. Huelamo, C. Pinte +15

In order to improve our understanding of substellar formation, we have performed a compositional and structural study of a brown dwarf disk. We present the result of photometric, s…

astro-ph2008★ 24 cited

Follow-up observations of binary ultra-cool dwarfs

H. Bouy, E. L. Martin, W. Brandner +12

Astrometric observations of resolved binaries provide estimates of orbital periods and will eventually lead to measurement of dynamical masses. Only a few very low mass star and br…

astro-ph2007★ 22 cited

Multi-Conjugate Adaptive Optics images of the Trapezium Cluster

H. Bouy, J. Kolb, E. Marchetti +3

Multi-Conjugate Adaptive Optics (MCAO) combines the advantages of standard adaptive optics, which provides high contrast and high spatial resolution, and of wide field ~1' imaging.…