Lyα Absorption‐Line Systems in the Gravitational Lens Q0957+561

Autor: P. T. Boyd, Jeffrey W. Percival, Joseph F. Dolan, Frederick C. Bruhweiler, Andrew G. Michalitsianos, Robert J. Hill, M. J. Nelson, Demos Kazanas, G. W. van Citters
Rok vydání: 1997
Předmět:
Zdroj: The Astrophysical Journal. 474:598-605
ISSN: 1538-4357
0004-637X
DOI: 10.1086/303491
Popis: Far-ultraviolet spectra of the gravitational lens components Q0957+561A and B were obtained with the Hubble Space Telescope Faint Object Spectrograph (HST FOS). Two previously known absorption-line systems were detected at redshifts zdamped = 1.3911 and zLyα = 1.1249. Their prominent absorption features are superposed on intense QSO continuum emission between λλ900-1400 in the quasar rest frame. Strong O VI λ1033, Lyα λ1216, and N V λ1240 line emission found at the QSO redshift (zQSO = 1.41) accompany the absorption-line systems. Lyα through Ly associated with the damped absorption system were found in both lensed components, together with other ionic species of N I, N III, C II, C III, Si II, Si III, and O I. We tentatively identify O VI λλ1033, 1037 absorption at the damped Lyα redshift, which, if confirmed, would be the highest ionization species yet detected in such systems. The equivalent widths of the Lyman series in Q0957+561A are measurably greater compared with absorption in 0957+561B, consistent with the narrower and shallower depth of the Lyman series line profiles in image B. The differences of the damped Lyman series absorption in the lensed components are the only significant spectral characteristic that distinguishes the far-ultraviolet spectra of 0957+561A and B. These results indicate that the damped Lyα absorber is inhomogeneous over scale lengths of ~200 pc, which corresponds to the beam separation at the damped Lyα redshift. However, the equivalent widths of neutral and ionized metals in lens components A and B are correlated, which suggests these spectral features arise in an extended region. The metal line-absorption strength is consistent with lower column densities compared with the hydrogen line-forming region. Thus, the small coherence length scale indicated by the difference in hydrogen line absorption between the lensed components suggests the geometric ray paths intercept different regions of a galactic disk that is viewed pole-on, while the metal absorption occurs in the halo.
Databáze: OpenAIRE
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