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Distances, Luminosities, and Temperatures of the Coldest Known Substellar Objects

Science  05 Sep 2013:

DOI: 10.1126/science.1241917

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Abstract

The coolest known brown dwarfs are our best analogs to extrasolar gas-giant planets. The prolific detections of such cold substellar objects in the past two years have spurred intensive followup, but the lack of accurate distances is a key gap in our understanding. We present a large sample of precise distances based on homogeneous mid-infrared astrometry that robustly establish absolute fluxes, luminosities, and temperatures. The coolest brown dwarfs has temperatures of 400 to 450 kelvin and masses ≈ 5 to 20× that of Jupiter, showing that they bridge the gap between hotter brown dwarfs and gas-giant planets. At these extremes, spectral energy distributions no longer follow a simple correspondence with temperature, suggesting an increasing role of other physical parameters such as surface gravity, vertical mixing, clouds, and metallicity.

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