D. Stathopoulos scite author profile

Most of the Broad Absorption Lines (BALs) in quasars show very complex profiles. An idea to explain these profiles is that the dynamical systems of broad line regions are not homogeneous but consist of a number of dense regions or ion populations with different physical parameters. This approach is used to study the ultraviolet CIV resonance lines in the spectra of a group of high ionization BAL quasars, using the Gauss-Rotation model.

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A statistical study of C IV regions in 20 Oe-stars

Antoniou

Danezis

Lyratzi

et al. 2014

Advances in Space Research

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D. Stathopoulos

On Si ivand C ivbroad absorption line variability in the UV spectra of 10 BALQSOs

Investigating the reasons of variability in Si IV and C IV broad absorption line troughs of quasars

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The Complex Broad Absorption Line Profiles in a Sample of QSO Spectra

A statistical study of C IV regions in 20 Oe-stars

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