In astronomy, a RAMBO or robust association of massive baryonic objects is a dark cluster made of brown dwarfs or white dwarfs.
RAMBOs were proposed by Moore and Silk in 1995. They may have an effective radius between 1 and 15 pc, with masses in the range 10–100,000 M ⊙ {\displaystyle M_{\odot }} (solar masses).
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