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With a distance of 1/2 of the star separation, you don't get stable orbits around a single star. I think I read something about of 1/7 of the star separation for stable (and nearly circular) orbits.
Gas giant with close orbits should be possible due to orbital mechanics, but I think they would have been visible in the radial velocity measurements (did not check the numbers).
Gas giant with close orbits should be possible due to orbital mechanics, but I think they would have been visible in the radial velocity measurements (did not check the numbers).