ISIS Spectrum of Teide 1
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ISIS Spectrum of Teide 1

ISIS Spectrum of Teide 1

The optical spectrum of Teide 1 (upper trace) and of the M9 dwarf LHS 2065 (lower trace). The flux scale of both spectra is normalized to unity at 825 nm. An offset has been added to the spectrum of Teide 1 for clarity. This spectrum confirmed the discovery of the coldest quasi-stellar object known in the Universe, the brown dwarf Teide 1. The spectral lines of neutral potasium between 767-770 nm indicated that it was an object with high surface gravity, as was expected for a brown dwarf, and the presence of prominent bands of titanium oxide and, espcially, vanadium oxide at 750 nm allowed to derive its spectral classification and an estimate of its effective surface temperature, which turned out to be some 2350 K. [TIFF]



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Last modified: 13 December 2010