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- W173008927 abstract "One of the characteristics of quasars is the presence of strong emission lines in their spectra. There are broad and narrow lines indicating broad and narrow line emitting regions (BLR and NLR, respectively). Beside these two regions, a very broad Fe Kα line is often present in the X-ray spectral band. Additionally, in the UV spectral band, the broad absorption line components are present in a fraction of 10% of quasars. Here we give a short overview of investigation of line shapes and their use to diagnose the plasma physics and kinematics in quasar emitting regions." @default.
- W173008927 created "2016-06-24" @default.
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- W173008927 date "2010-01-01" @default.
- W173008927 modified "2023-10-01" @default.
- W173008927 title "Spectral line shapes as a tool for investigation of kinematics and physics of plasma in quasars." @default.
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