Metal-line system at z=2.18 in quasar system

This image shows lines from a metal-line system at redshift z = 2.18 towards HE22-28.

Although the Lyman-alpha absorption line (bottom) shows only one component, with the metal lines blueshifted by ~ 40 km/sec, the corresponding Lyman-beta line (the observed wavelength is 326 nm near the atmospheric cut-off!) reveals that the complex consists of two components (clouds), separated by ~ 83 km/sec, at z = 2.1795 and at z = 2.1804.

The Voigt profile fitting gives a total column density of N(HI) = 1.3 x 10 16 cm -2 and accurate values for the column densities of SiIV, SiII, CIV, SiIII and CII. The SiIV/CIV ratio, an indicator of the temperature of the ionizing background for the z = 2.1795 component gives ~ 0.23 which is similar to what has been found in higher-z systems, suggesting little evolution in the shape of the spectrum of the ionizing background .

Mynd/Myndskeið:

ESO

Um myndina

Auðkenni:eso0013h
Tegund:Skýringarmynd
Útgáfudagur:6. apríl 2000
Tengdar fréttatilkynningar:eso0013
Stærð:520 x 712 px

Um fyrirbærið

Nafn:QSO HE22-28
Tegund:Early Universe : Galaxy : Activity : AGN : Quasar
Fjarlægð:z=2.4 (rauðvik)
Flokkur:Quasars and Black Holes

Myndasnið

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