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HS 1603+3820: a bright z(em)=2.51 quasar with a very rich heavy element absorption spectrum

A. Dobrzycki·D. Engels·H. -J. Hagen
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Abstract

During the course of Hamburg/CfA Bright Quasar Survey we discovered a bright (B=15.9), high redshift (z=2.51) quasar HS 1603+3820. The quasar has a rich complex of CIV absorbers, containing at least five systems, all within 3000 km/s from one another. Despite large ejection velocity (v(ej)>5000 km/s for all components) the complex is likely to be associated with the quasar. There are at least three more associated heavy element absorbers, two of which have z(abs)>z(em). Together, they make one of the richest known complexes of associated heavy element absorbers, and the richest in objects with B<16. The combination of redshift, brightness, richness of the metal absorption spectrum and richness of the associated absorption is unmatched among known quasars.

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A. Dobrzycki, D. Engels, H. -J. Hagen. 1999-08-12. HS 1603+3820: a bright z(em)=2.51 quasar with a very rich heavy element absorption spectrum. https://arxiv.org/abs/astro-ph/9908134

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