New SpeX Observations of M7-L6 Dwarfs
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https://b2find.eudat.eu/dataset/20207734-0e0e-5d42-a19f-a18fc1f8bd1d
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Multiplicity is a key statistic for understanding the formation of very low mass (VLM) stars and brown dwarfs. Currently, the separation distribution of VLM binaries remains...
