This is the final version. Available on open access from the American Astronomical Society via the links in this recordThe detection of brown dwarfs in globular star clusters will allow us to break the degeneracies in age, mass and composition that affect our current models, and therefore to constrain the physics of their atmospheres and interiors. Furthermore, detecting brown dwarfs will help us constrain the properties of the clusters themselves, as they carry information about the clusters' age and dynamics. Great advancements in this field are to be expected in the next ten years, thanks to the extraordinary sensitivity in the infrared of upcoming telescopes like JWST and the ELTs
This paper discusses benchmark brown dwarfs in various environments, and focuses on those in wide bi...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
We review the current picture of disks around cool stars and brown dwarfs, including disk fractions,...
We present an analysis of the second epoch Hubble Space TelescopeWide Field Camera 3 F110W near-infr...
‘The definitive version is available at www3.interscience.wiley.com '. Copyright Royal Astronomical ...
Brown dwarfs can serve as both clocks and chemical tracers of the evolutionary history of the Milky ...
International audienceThe initial mass function is an important key to understand star formation pro...
Evolutionary models of brown dwarfs are plagued by a lack of observational constraints. The complex ...
ChH highlights financial support of the European Community under the FP7 by an ERC starting grant. S...
We present a sample of brown dwarfs identified with the Wide-field Infrared Survey Explorer (WISE) f...
Brown dwarfs are objects with sub-stellar masses that are unable to sustain hydrogen burning, coolin...
This thesis describes the search for brown dwarfs in open clusters using optical and infrared photom...
We know a lot about stars and planets. We know about stars because they are easy to detect and beca...
Brown dwarfs are objects with sub-stellar masses that are unable to sustain hydrogen burning, coolin...
The multiplicity properties of brown dwarfs are critical empirical constraints for formation theorie...
This paper discusses benchmark brown dwarfs in various environments, and focuses on those in wide bi...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
We review the current picture of disks around cool stars and brown dwarfs, including disk fractions,...
We present an analysis of the second epoch Hubble Space TelescopeWide Field Camera 3 F110W near-infr...
‘The definitive version is available at www3.interscience.wiley.com '. Copyright Royal Astronomical ...
Brown dwarfs can serve as both clocks and chemical tracers of the evolutionary history of the Milky ...
International audienceThe initial mass function is an important key to understand star formation pro...
Evolutionary models of brown dwarfs are plagued by a lack of observational constraints. The complex ...
ChH highlights financial support of the European Community under the FP7 by an ERC starting grant. S...
We present a sample of brown dwarfs identified with the Wide-field Infrared Survey Explorer (WISE) f...
Brown dwarfs are objects with sub-stellar masses that are unable to sustain hydrogen burning, coolin...
This thesis describes the search for brown dwarfs in open clusters using optical and infrared photom...
We know a lot about stars and planets. We know about stars because they are easy to detect and beca...
Brown dwarfs are objects with sub-stellar masses that are unable to sustain hydrogen burning, coolin...
The multiplicity properties of brown dwarfs are critical empirical constraints for formation theorie...
This paper discusses benchmark brown dwarfs in various environments, and focuses on those in wide bi...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society....
We review the current picture of disks around cool stars and brown dwarfs, including disk fractions,...