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WISEPA J062309.94-045624.6
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WISEPA J062309.94−045624.6 is a brown dwarf of spectral type T8. It is the coldest, and latest spectral type brown dwarf observed to produce radio emission.
Very Large Telescope image of WISE J0623−0456
Very Large Telescope image of WISE J0623−0456
L dwarf
Videos
An object with the spectral type L can be either a low-mass star, a brown dwarf or a young free-floating planetary-mass object. If a young exoplanet or planetary-mass companion is detected via direct
Spectrum of Kelu-1 (L-type binary, bottom line) in comparison to an M6-dwarf, which shows much stronger TiO and sodium absorption.
Spectrum of Kelu-1 (L-type binary, bottom line) in comparison to an M6-dwarf, which shows much stronger TiO and sodium absorption.
The L-type binary CWISE J0146-0508AB (L4+L8 blue)
The L-type binary CWISE J0146-0508AB (L4+L8 blue)