Formation of galaxy clusters corresponds to the collapse of the largest gravitationally bound
overdensities in the initial density field and is accompanied by the most energetic …

The density distribution arising at the nonlinear stage of gravitational instability is similar to
intermittency phenomena in acoustic turbulence. Initially small-amplitude density …

We present emission-line measurements and physical interpretations for a sample of 117 [O
iii] emitting galaxies at z= 5.33–6.93, using the first deep JWST/NIRCam wide-field slitless …

The evolution of large-scale structure in a universe dominated by cold dark matt ADS Classic is
now deprecated. It will be completely retired in October 2019. This page will automatically …

Kenneth Lang's classic work Astrophysical Formulae.(Vol. I and II) is now available as soft
cover edition in a set. This volume is a reference source of fundamental formulae in physics …

A standard sample for the comparison of the HI content of galaxies in various intergalactic
environments is presently defined by means of observations of 324 isolated galaxies lying in …

We describe an attempt to reconstruct the initial conditions for the formation of cosmological
large-scale structure, under the assumption of gravitational instability in a Gaussian density …

We review the quantitative science that can be and has been done with redshift and peculiar
velocity surveys of galaxies in the nearby universe. After a brief background setting the …

Recent observations indicate that most galaxies are concentrated in superclusters
consisting of galaxies, and clusters of galaxies, aligned along strings. Giant volumes exist …

A catalog of rich clusters of galaxies ADS Classic is now deprecated. It will be completely retired
in October 2019. This page will automatically redirect to the new ADS interface at that point …