There's no need to get all angry here. The answers so far provided were accurate, even if not exactly on the exhaustive side.
You basically asked two questions:
1. what does the presence of a supermassive black hole mean for the orbital motion of stars in a galaxy
2. what does the rotation of the black hole mean for the same
Re.1:
The orbital speed of a small object(like a star) depends on the mass of the object being orbited and distance from it, as per the Newton's laws. You get Kepler's laws from this.
It can be shown mathematically that, as long as its density is spherically symmetrical, it doesn't matter how big(spatially extensive) is the central object(
http://en.wikipedia.org/wiki/Shell_theorem). Only the mass matters. For the purposes of calculating orbits, all massive objects can be treated as if all of their mass was concentrated in a point at their centre.
That's why the fact of there being a 1 million solar masses black hole in the centre of the galaxy is irrelevant outside its immediate neghbourhood. Its gravitational field looks exactly the same as if there were 1 million stars packed in a roughly spherical distribution.
And that's not even such a huge number, considering ~100 billion stars the Milky Way contains.
As Vanadium said, it could be even 1 million solar masses of feathers, and the orbits of far away stars would look just the same.
The only difference it makes is for the stars very close to the black hole, which do orbit faster than if they were surrounded by other stars - this is also explained by the shell theorem(the second part in the wiki article) - and which are affected by tidal forces raised by the concentrated mass of the black hole.
Re.2:
For the rotation of a massive body to have any effect on other bodies, it'd have to somehow drag the space around it. General Relativity predicts such an effect:
http://en.wikipedia.org/wiki/Frame_dragging . However, it is very tiny, so from the point of view of the stars in the galaxy it's negligible. For all they care, the black hole may just as well not spin at all, or spin in the opposite direction.Re: the post above this one:
- Whenever you say "magnetism" in that post, you ought to say "gravity". It doesn't make sense otherwise.
- Galaxies spin because of the conservation of momentum of the collapsing gas from which they coalesced. One direction emerges during the collapse and is further magnified the further it goes. Just as with stellar systems or water going down the drain.
Here's a simulation of such a collapse, made by the guys from Univ. of Zurich:
- Galaxies move in the intergalactic space according to the conservation of linear momentum and gravitational attractions with other galaxies. Whether there is or isn't a black hole in the centre doesn't matter.Finally, as an interesting aside, the measured velocities of stars in galaxies appear to conflict with the velocities predicted by analysing the distribution of visible mass. This has led to the introduction of the concept of Dark Matter to explain the discrepancies.