  The work is devoted to the construction of explicit embeddings for the
metrics of the black holes, formed by nonsingular matter distribution. One of
the possible examples of such type of solutions is regular black hole. Using
the existing classification of minimal symmetric embeddings of the
Schwarzschild metric as a base, we construct embeddings for regular black holes
with de Sitter interior. Another simple example is black hole, formed by
collapsing homogeneous spherically symmetric cloud of dustlike matter. We
discuss embeddings for two variants of such black holes - the one with the
eternally existing horizon, when dust ball never leaves the interior of the
horizon, and another variant with the dynamically forming horizon.
