Brown Dwarfs
After a discussion of the physical processes in brown dwarfs, we present a complete, precise definition of brown dwarfs and
299 indexed results
After a discussion of the physical processes in brown dwarfs, we present a complete, precise definition of brown dwarfs and
We discuss a scenario in which brown dwarfs are formed like stars, except that their full collapse phases are interrupted
The origin of brown dwarfs (BDs) is an important component of the theory of star formation, because BDs are approximately
An area large enough (180 sq arcmin) to put constraints on a possible low mass brown dwarf population in the
We have obtained deep CCD R and I mosaic imaging of 578 arcmin$^{2}$ within 1$^{\circ}$.5 of the Pleiades' center --
We have obtained near-IR observations of some of the faintest objects so far known towards the Pleiades cluster, with the
The brown dwarf population in the Pleiades cluster has been probed in a deep 850 arcmin2 RIJK survey. The survey
AA Dor is an eclipsing, close, post common-envelope binary consisting of a sdOB primary star and an unseen secondary with
We describe a unique mass determination for a microlensing event from the second phase of the Optical Gravitational Microlensing Experiment
We have developed a new non-gray theory of the evolution, spectra, and colors of extrasolar giant planets (EGPs) and brown
Brown dwarfs may have such low masses because they are prematurely ejected from small unstable multiple systems, while the members
I summarize some of the consequences for the optical and very-near-infrared spectra of T dwarfs (in particular) and brown dwarfs
HD10697 is a nearby main-sequence star around which a planet candidate has recently been discovered by means of radial-velocity measurements
We analyzed the Hipparcos astrometric observations of 47 stars that were discovered to harbor giant planets and 14 stars with
Studies of disks around young brown dwarfs are of paramount importance to our understanding of the origin, diversity and early
We are conducting a U,B,R,I monitoring program to identify pre-main sequence stars and brown dwarfs in a 12.5x12.2 square degree
We have undertaken a differential photometric I band search for variability in three Pleiades brown dwarfs and three very low
We report VLT/NACO imaging observations of the stars GSC 08047-00232 and HIP 6856, probable members of the large Tucana-Horologium association.
Brown dwarfs, which straddle the mass range between stars and planets, appear to be common both in the solar neighborhood
Observations of brown dwarfs provide important feedback on theories of atmospheres and inner structure of substellar objects. Brown dwarf binary
AB Dor C, a low-mass companion to the young star AB Dor A has recently been imaged. Direct detection and
The presence of brown dwarfs in the dark galactic halo could be detected through their gravitational lensing effect and experiments
We report the discovery of an isolated brown dwarf with similar properties to the binary object Gliese 229B and to
Brown dwarfs are classified as objects which are not massive enough to sustain nuclear fusion of hydrogen, and are distinguished