The spectrum from an accretion disk consisting of multiple blackbody components. For example, see Mitsuda et al. (1984) or Makishima et al. (1986).
|par1||temperature at inner disk radius (keV)|
|norm||, where where is “an apparent” inner disk radius in km, the distance to the source in units of 10 kpc, and the angle of the disk ( is face-on). On the correction factor between the apparent inner disk radius and the realistic radius, see e.g., Kubota et al. (1998).|