Radiation spectra of warm and optically thick coronae in agns

HIGHLIGHTS

• who: Petrucci P.-O. et al. from the UnivGrenoble Alpes, CNRS, IPAG, Grenoble, France have published the research work: Radiation spectra of warm and optically thick coronae in AGNs, in the Journal: (JOURNAL)
• what: The aim of this paper is to simulate energy-dependent spectra of warm coronae in radiative equilibrium thanks to the state-of-the-art radiative transfer code titan coupled with the Monte-Carlo code noar (Dumont et_al 2003). To ease the analysis, the authors adopt here a number of simplifying assumptions with respect to the numerical calculations described in the following . . .
  

   

  

  If you want to have access to all the content you need to log in!

  Thanks :)

  Username or E-mail:

  If you don't have an account, you can create one here.