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Detection of Debris Disks and Wide Orbit Planets with the LBTI

Authors: Philip M. Hinz; Tomonori Usuda; Motohide Tamura; Miki Ishii;

Detection of Debris Disks and Wide Orbit Planets with the LBTI

Abstract

The Large Binocular Telescope Interferometer (LBTI) is designed to probe nearby stars for dust disks, indicative of planetesimal belts, as well as giant planets in wide orbits (>3 AU). The instrument provides a unique combination of resolution and sensitivity in the thermal infrared to achieve these objectives. Both of these programs will provide important insights into the architecture for other planetary systems. The discovery space of the LBTI is presented, as well as recent observational results from prototype instruments now being carried out at the MMT Observatory.

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Powered by OpenAIRE graph
Found an issue? Give us feedback
selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
4
Average
Average
Average
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