Weeeelll... Just some interesting stipulations:
Radiation power weakens by square of the distance, ie. if you go to double the distance, you get one fourth of the power from the star.
This means that if you have a star with absolute magnitude of 25 Suns, the habitable zone would be about 5 AU from thestar - AND the habitable zone would be about five times as wide as the one around Sun.
That means that chances for having a planet on stable habitable zone orbit around two stars that orbit each other go drastically low. The stars would need to be orbiting each other very close to each other and be bright enough to support habitable zone at a distance that isn't too badly disturbed with the gravitational oscillations (also called tides by the way) from the rotating system of two gravitational bodies, but if that would work out, then the system could be stable. Assuming that no other star from the system will pass close by and disrupt everything.
The other possibility is more interesting one.
If you have a star that has 0.01 times the brightness of the Sun (ie. red dwarf), the habitable zone is found at about 0.1 AU from the star. That's a minuscule distance at solar scale; it would with very high probability allow a red dwarf in multiple star system to retain planets around it on stable orbits; some could be on the habitable zone.
Same applies to all multiple star systems with stars (like Galaxies! we have a 100 billion star system right there!) at sufficient distance from each other - each star could, with more or less ease, have stable planetary orbits on the habitable zone.

...yes, I know that with multiple star system, the definition is that the stars all orbit a local center of gravity, ie. each other.
This is an interesting toy. Try out the Four-mutual orbit - if each were a star, each could have planets around them, and each of them could have moons on stable orbits. If the mentioned orbits were close enough to the star, that is.