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we do know that x-ray binaries give off mostly x-rays its sort of a problem for people who are interested in them because there are a lot of other objects that give off x-rays that we can see in the sky and then we can often get them confused for x-ray binaries and so what we have to do is look at the object and at particular x-ray object at other wavelengths so as you go from the x-rays and you go towards the ultraviolet part of the accretion disk around an x-ray binary can be hot enough that it it will be very bright in the ultraviolet compared to other kinds of x-ray emitting sources the accretion disk may also have a component in the optical so light that we can see and then as you move to longer wavelengths typically what youll see with sort of an ordinary stellar companion is that at a certain point you wont be seeing light from the compact object or from the disc you will be seeing light from the companion star itself and the companion stars light can stretch into the infra