MIR-Imaging brown dwarfs in binary systems with ESO/VLT and Gemini

Details MIR-Imaging brown dwarfs in binary systems with ESO/VLT and Gemini MIR-Imaging brown dwarfs in binary systems with ESO/VLT and Gemini

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20923808s&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #238.08; Bulletin of the American Astronomical Society,

Astronomy and Astrophysics

Astronomy

Scientific paper

Diffraction-limited mid-infrared imaging is required to resolve individual components in close low-mass binary or multiple systems in order to constrain their atmospheres or circumstellar disks.
Gemini(T-Recs) and VLT(VISIR) demonstrate the power of high-sensitivity, high-spatial resolution ground-based MIR observations of brown dwarfs binaries. I will highlight recent results where differential MIR photometry allows to probe the cool atmospheres of the nearby brown dwarf binary eps Indi B, and the disks around several young, nearby, very-low mass, objects.

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