I'm having some trouble understanding what is going on in Mathematical methods of classical mechanics (Arnold, 2nd edition) in the rigid body mechanics section (chapter 6). I don't know any other book that deals with rigid body mechanics like this. After introducing two frames of reference: the "stationary" one $k$ and the "moving" one $K$, he defines an operator \begin{equation} B:K\rightarrow k \end{equation} That turns vectors from one space into vectors of the other.
Then, after defining the angular velocity $\boldsymbol{\omega}$ (vector in $k$), he defines the angular velocity of the body as: \begin{equation} \boldsymbol{\Omega}=B^{-1}\boldsymbol{\omega} \end{equation} (vector in $K$). This is the first time I see such distinction. Why?
Anyways, I think it's fine up to this. The problems start to rise when he deals with rigid bodies and chooses $K$ as the "system rotating together with the rigid body", with respect to which the body is stationary (see Inertia operator section, page 136-137).
If it is so, then how does it have an angular momentum $\boldsymbol{M}$ in $K$ (its points should have zero velocity $\boldsymbol{V}$ in that system, since it's rotating together with the body). What am I missing?