Prior editions have established the basics, in terms of how many gas giants and planetoid belts are present, and what the star's type is. For the star type I'd use the TNE version of any published sector (for TNE that includes the Marches), as TNE corrected a couple early misconceptions about star types and their frequency, and relegated most dwarf stars to companion positions in the interest of having livable worlds in this big space opera of ours.
For example, you'll see a line like this:
Vilis 1119 A593943-A Hi In 820 Im G5 V M8 D
The '820' indicates the population multiple (8 billion people in this case), the number of planetoid belts in-system (two), and the number of gas giants (none). Planetoid belts are *in addition* to an Asteroid belt main world, should that be the case.
This system is a binary, with a mid-yellow main sequence star (Sol is a G3 V), and a late, cool, red dwarf companion.
The relationship of the two stars is not defined, and could be anything from close (orbit zero, basically) to a far companion (potentially has its own planets, burnt out rock balls though they may be) or anything in between.
The above line is pulled from the TravellerWiki, by the way, which, being a Wiki, is suspect. In this case, the data for Vilis matches the MegaTraveller data, and the stars are not the type that would have seen a TNE revision.