Evolution of the Clustering of QSO Absorbers from Redshifts 4 to 0

Details Evolution of the Clustering of QSO Absorbers from Redshifts 4 to 0 Evolution of the Clustering of QSO Absorbers from Redshifts 4 to 0

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aas...193.8506q&link_type=abstract

American Astronomical Society, 193rd AAS Meeting, #85.06; Bulletin of the American Astronomical Society, Vol. 30, p.1379

Astronomy and Astrophysics

Astronomy

Scientific paper

We extend our QSO absorber clustering program by comparing the correlation function of a new sample of low-redshift heavy-element absorbers with that which we previously obtained for higher-redshift absorbers. We are thus able to trace the evolution of the clustering of absorbers from redshifts of over 4 to 0, and on scales from about 1 to 100 comoving Mpc. The implications for cosmology and growth of structure via gravitational instability are discussed.

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