Study of the C IV ($\lambda\lambda$1548.187 - 1550.772), Si IV ($\lambda\lambda$1393.755 - 1402.770) and O IV ($\lambda$1401.156) Regions of the QSO J021327.25-001446.93

A. Antoniou; Ch. Katsavrias; E. Danezis

arxiv: 1405.3276 · v1 · pith:GIYCAQP4new · submitted 2014-05-13 · 🌌 astro-ph.GA

Study of the C IV (λλ1548.187 - 1550.772), Si IV (λλ1393.755 - 1402.770) and O IV (λ1401.156) Regions of the QSO J021327.25-001446.93

Ch. Katsavrias , E. Danezis , A. Antoniou This is my paper

classification 🌌 astro-ph.GA

keywords lambdaregionsabsorbingabsorptionanalyzebalrbroadcertain

0 comments

read the original abstract

Broad Absorption Line Regions - BALR are composed of a number of successive independent absorbing density layers. Using the GR model, we analyze the UV Si IV ({\lambda}{\lambda}1393.755 - 1402.770), O IV ({\lambda}1401.156) and C IV ({\lambda}{\lambda}1548.187 - 1550.772) resonance lines in the spectra of a certain QSO and discuss the results concerning its kinematic properties (rotational, radial and random velocities).

This paper has not been read by Pith yet.

Study of the C IV (λλ1548.187 - 1550.772), Si IV (λλ1393.755 - 1402.770) and O IV (λ1401.156) Regions of the QSO J021327.25-001446.93

discussion (0)