17 4 v 1 1 0 A pr 2 00 2 Two-temperature coronal flow above a thin disk

@inproceedings{Liu2002174V,
  title={17 4 v 1 1 0 A pr 2 00 2 Two-temperature coronal flow above a thin disk},
  author={Bo Liu and E. Meyer-Hofmeister and Toshihiro Kawaguchi},
  year={2002}
}
We extended the disk corona modelHofmeister 2000a) to the inner region of galactic nuclei by including different temperatures in ions and electrons as well as Compton cooling. We found that the mass evaporation rate and hence the fraction of accretion energy released in the corona depend strongly on the rate of incoming mass flow from outer edge of the disk… CONTINUE READING