Clusters of galaxies are gravitationally bound configurations containing typically hundreds of
galaxies in a region about 10 25 cm in size. They range from irregular clusters, with strong …

The authors present results from HI synthesis observations and optical surface photometry of
four dwarf irregular galaxies within the Virgo Cluster. HI distributions and rotation curves …

The dynamics of the Coma cluster are probed through the study of spiral galaxies that have
been stripped of gas and ellipticals that have been tidally stripped. Since such stripping is …

The Spartan 1 instrument has resolved the spatial and spectral distribution of the 1-10 keV X-
ray emission from the Perseus cluster in a region extending 50'(1.6 Mpc) from the center …

Mixing of dynamically swept galaxy and cluster gas, so as to render one-fluid calculations
completely reliable, is sufficient only if the flow Mach number is much smaller than one. The …

Nonlinear Shear Instabilities in an Infinite Slab ADS Classic is now deprecated. It will be
completely retired in October 2019. This page will automatically redirect to the new ADS interface …

The calculations presented suggest that the material stripped from galaxies and gathered in
wakes in a rich cluster can only begin to mix efficiently with the surroundings if galaxies …

The Spartan 1 instrument has resolved the spatial and spectral distribution of the 1–10 keV
X-ray emission from the Perseus cluster in a region extending 50'(1.6 Mpc) from the center …

9.3 Galaxies with special peculiarities; pairs, groups and clusters of galaxies (P. Biermann);
9.3.6 References for 9.3, pp. 2 Page 1 9.3.6 References for 9.3 279 9.3.6 References for 9.3 …

9.3 Galaxies with special peculiarities; pairs, groups and clusters of galaxies (P. Biermann);
9.3.5 Superclusters, p. 278 Page 1 278 9.3.5 Superclusters [Ref. p. 279 can be understood [S …