  The catalog of hierarchical stellar systems with three or more components is
an update of the original 1997 version of the MSC. For two thousand
hierarchies, the new MSC provides distances, component's masses and periods, as
well as supplementary information (astrometry, photometry, identifiers, orbits,
notes). The MSC content and format are explained, its incompleteness and strong
observational selection are stressed. Nevertheless, the MSC can be used for
statistical studies and it is a valuable source for planning observations of
multiple stars. Rare classes of stellar hierarchies found in the MSC (with 6 or
7 components, extremely eccentric orbits, planar and possibly resonant orbits,
hosting planets) are briefly presented. High-order hierarchies have smaller
velocity dispersion compared to triples and are often associated with moving
groups. The paper concludes by the analysis of the ratio of periods and
separations between inner and outer subsystems. In wide hierarchies, the ratio
of semimajor axes, estimated statistically, is distributed between 3 and 300,
with no evidence of dynamically unstable systems.
