Can we assume that most (if not all) black holes are rotating, due to conservation of momentum?
I am excluding the micro world from this question, just thinking of the range of stars on the main sequence of the H-R diagram as they shrink over time.
Can anyone give me an example of non-rotating macro sized B.H., e.g a binary system where each star counter-rotates relative to the other and explain how they may, (if they can) at least slow down each others's rotational velocity?