Originally posted by Nereid
If they were truly isolated, it's hard to imagine how they'd be detected, other than by gravitational lensing.
The one that best meets your criterion is the supermassive one at the centre of our Milky Way galaxy - we know it's there, how massive it is, etc, yet there are no accretion disks, jets, etc. Of course, if by 'companion stars' you mean stars orbiting about a BH, then we're such a companion (although there's an awful lot more mass than just the galactic BH which contributes to our motion).
This link gives you an idea of how 'alone' the Milky Way centre BH is:
http://www.eso.org/outreach/press-rel/pr-2002/pr-17-02.html