Quote:
Originally Posted by weby
I have not followed the latest developments so I could be wrong on that, but back when I last read about them the mass of brown dwarf disks was thought to be much less than that of disks around "real" stars. And if I remember correctly that was the reason/one of the reasons for the low count of gas giants around them.
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My "evidence" is mostly "a few hours with google/wikipedia", so take anything I say with a heavy dose of salt.