Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...326..710j&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 326, March 15, 1988, p. 710-716.
Astronomy and Astrophysics
Astrophysics
10
Absorption Spectra, Astronomical Spectroscopy, Galactic Clusters, Quasars, Emission Spectra, Red Shift
Scientific paper
Four faint quasar candidates surrounding the wide quasar pair Tololo 1037-271/1038-272 have been observed with the aim of searching for absorption due to the intervening supercluster proposed to explain the strong correlated absorption seen between z = 1.95 and z = 2.15 in these two objects. A potential positive detection is reported in the case of Tol 1035-276, located at z(em) = 2.15, 39 arcmin southwest of the pair. Both the emission redshift of this object and two of the absorption systems seen in its spectrum match corresponding systems in Tol 1035-271/1038-272 to an accuracy well within the velocity splitting expected from the Hubble expansion at the large angular separation. In contrast, no correlated absorption is detected at a larger separation in the spectrum of Tol 1033-269 located at z(em) = 2.42, 62 arcmin west of the pair. This may indicate that the intervening supercluster has an elongated shape with its largest dimension aligned with the line of sight.
Cristiani Stefano
Jakobsen Peter
Perryman Michael . A. C.
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