Our inferred
debris disc model is able to reproduce G196 - 3B's spectral energy distribution to a satisfactory level of achievement.
We present the first far - infrared spatially resolved images of these discs and new single - component
debris disc models.
Not exact matches
The researchers
modeled the resulting accretion
disc — an elliptical
disc of stellar
debris swirling around the black hole — along with its probable speed, radius, and rate of infall, or speed at which material falls onto the black hole.
By using
models of how planets shape a
debris disc, the team found that «eccentric» versions of the giant planets in the outer solar system could explain the observed properties of the ring.
In our
models we consider collisions, direct radiation pressure, and drag forces, i.e. the actual physical processes operating in
debris discs.
Our
models are compared to a suite of observational data for thermal and scattered light emission, ranging from th... ▽ More The spatially resolved AU Mic
debris disc is among the most famous and best - studied
debris discs.