On outflowing viscous disc models for Be stars

@inproceedings{Porter1999OnOV,
  title={On outflowing viscous disc models for Be stars},
  author={John M. Porter},
  year={1999}
}
It is assumed that Be star discs are driven by viscosity. Emission from disc models is calculated and is confronted with continuum observations. It is found that the outflowing viscous disc models can reproduce the observed IR continuum emission. However, to exist as outflowingdiscs, either the discs are significantly acted upon by the stellar radiation… CONTINUE READING