Photometric Properties of L and T Dwarf Binaries
Abstract Recent studies using volume-limited samples of brown dwarfs have revealed the photometric evolution of single L and T dwarfs and unresolved binaries as they age and cool, in particular as they transition from L to T spectral types. We demonstrate that the near-infrared photometric evolution of the resolved components of L and T dwarf binaries is consistent with that of single objects using a volume-limited sample. In addition, we provide supporting evidence that the L9 dwarf WISE J185101.83+593508.6 is an unresolved binary and identify three more candidate or confirmed unresolved binaries all from being overluminous for their spectral type. We calculate a new binary fraction of 13.1% ± 1.8% for L0–T8 dwarfs.
2003 ◽
Vol 211
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pp. 83-86
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2020 ◽
Vol 496
(2)
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pp. 1757-1765
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2018 ◽
Vol 479
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pp. 2702-2727
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2021 ◽
2003 ◽
Vol 211
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pp. 181-182
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