Not sure if I got the masses right but using 9.62 solar masses and 0.92 solar masses for the black hole and the star respectively with a period of 185 days gives me a semi-major axis of 1.39 AU (using an orbital period calculator). If that's correct then this star is orbiting quite close to the black hole. Chances of it having any planets would be quite small although I suppose there could be planets orbiting the binary system at a large distance.
I don't speak astrophysicist but I think this part
> Common envelope evolution can only produce the system’s wide orbit under extreme and likely unphysical assumptions. Formation models involving triples or dynamical assembly in an open cluster may be more promising.
means that the black hole and star formed separately and the black hole later captured the star? Hopefully the star had no life bearing planets before that, that would have been a terrible fate.
I don't speak astrophysicist but I think this part
> Common envelope evolution can only produce the system’s wide orbit under extreme and likely unphysical assumptions. Formation models involving triples or dynamical assembly in an open cluster may be more promising.
means that the black hole and star formed separately and the black hole later captured the star? Hopefully the star had no life bearing planets before that, that would have been a terrible fate.