We present a short general overview of the main features of exotic models of
neutron stars, focusing on the structural and dynamical predictions derived
from them. In particular, we discuss the presence of ``normal'' quark matter
and Color-Flavor Locked (CFL) states, including their possible self-bound
versions, and mention some different proposals emerging from the study of QCD
microphysics. A connection with actual observed data is the main goal to be
addressed at this talk and along the meeting. It is demonstrated that exotic
equations of state are {\it not} soft if the vacuum contributions are large
enough, and argued that recent measurements of high pulsar masses ($M \geq 2
M_{\odot}$) create problems for {\it hadronic} models in which hyperons should
be present.Comment: 8 pages, 2 figures. To be published in the Proceedings of the
conference "Isolated Neutron Stars: from the Interior to the Surface" (April
24-28, 2006, London, UK), eds. D. Page, R. Turolla, & S. Zan