  We update the SMC, Bridge, and LMC catalogues of extended objects that were
constructed by members of our group from 1995 to 2000. In addition to the rich
subsequent literature for the previous classes, we now also include HI shells
and supershells. A total of 9305 objects were cross-identified, while our
previous catalogues amounted to 7900 entries, an increase of $\approx12%$. We
present the results in subcatalogues containing 1445 emission nebulae, 3740
star clusters, 3326 associations, and 794 HI shells and supershells. Angular
and apparent size distributions of the extended objects are analysed. We
conclude that the objects, in general, appear to respond to tidal effects
arising from the LMC, SMC, and Bridge. Number-density profiles extracted along
directions parallel and perpendicular to the LMC bar, can be described by two
exponential-disks. A single exponential-disk fits the equivalent SMC profiles.
Interestingly, when angular-averaged number-densities of most of the extended
objects are considered, the profiles of both Clouds do not follow an
exponential-disk. Rather, they are best described by a tidally-truncated,
core/halo profile, despite the fact that the Clouds are clearly disturbed
disks. On the other hand, the older star clusters taken isolately, distribute
as an exponential disk. The present catalogue is an important tool for the
unambiguous identification of previous objects in current CCD surveys and to
establish new findings.
