Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103..154r&link_type=abstract
Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, Feb. 1991, p. 154-159. Research supported by Corni
Astronomy and Astrophysics
Astronomy
10
Galactic Clusters, Quasars, Red Shift, Absorption Spectra, Astronomical Spectroscopy, Metallicity
Scientific paper
Studies of QSO absorption lines can be used to discover 'superclusters' of metal-line systems (thought to be associated with galaxies) at large redshift, analogous to the absorbers found in the field surrounding the southern pair Tol 1037/1038. The unique ability of QSO absorption lines to reveal modest columns of gas at high redshift allows a pencil-beam survey of interesting fields. By concentrating on QSOs with known, rich, metal-line absorption systems and searching catalogs for nearby QSOs lying behind the proposed clusters, a number of promising fields have been identified. Initial results from QSOs surrounding Q1303 + 308 support the BAL hypothesis for the absorption in this object. It is shown that further observations will be of substantial use in delineating the extent and overdensity of superclustering at redshifts z = 1-21.
Filippenko Alexei V.
Romani Roger W.
Steidel Charles C.
No associations
LandOfFree
Searching for high-redshift superclusters does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Searching for high-redshift superclusters, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Searching for high-redshift superclusters will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1318652