Image Details
Caption: Figure 16.
Spectra of 2MASS J04335245+2612548, KPNO 3, and KPNO 7 after subtraction of the continuum fit and division by the average continuum flux in the 8–13 μm region to highlight the 10 μm silicate emission feature. These are the brown dwarfs for which we detect silicate emission as opposed to the results in Riaz (2009).
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