Clustering in networks with the collapsed Stochastic Block Model

Clustering in the Zel'dovich approximation

Clustering of galaxy clusters. II - Rare events in the cluster distribution

Clustering paradigms and multifractal measures

Clustering properties of galaxies - an empirical model

ClustOfVar: An R Package for the Clustering of Variables

CMB quadrupole induced polarisation from large scale structure.

CMB: polarization and temperature waves from spatially limited cosmological structures

CME Evolution in the Corona and Solar Wind

CMEs ‘en rafale’ observations and simulations

CN 1-1 - A peculiar compact planetary nebula

CN and CH variations among red giants in the globular cluster NGC 6171

CNO abundances and hydrodynamic models of the nova outburst. II - 1.00 solar mass models with enhanced carbon and oxygen

CO line emission from shock waves in molecular clouds

CO line formation in bipolar flows. II - Decelerated outflow case and summary of results

CO line formation in bipolar flows. III - The energetics of molecular flows and ionized winds

Coalescence Of 2, 3, Or More, Of Approx. 15 Heat Sources (Sustained By Radioactive Decay) Migrating Over Earth's Solid Inner Core Boundary, When Located Near Rotation Axis, In N- Or S-Hemisphere, Engenders Geomagnetic Field Reversals.

Coalescence of Black Hole-Neutron Star Binaries

Coalescence of self-gravitating gaseous masses - A numerical model

Coalescing binary neutron stars