  In this chapter we review the properties of the Orion outlying clouds at b <
-21 degrees. These clouds are located far off the Orion giant molecular cloud
complex and are in most cases small cometary-shaped clouds, with their head
pointing back towards the main Orion clouds. A wealth of data indicate that
star formation is ongoing in many of these clouds. The star formation in these
regions might have been triggered due to the strong impact of the massive stars
in the Orion OB association. Some of the clouds discussed here may be part of
the Orion-Eridanus bubble. An overview on each individual cloud is given. A
synthesis of the Pre-Main Sequence stars discovered in these clouds is
presented. We also discuss the millimeter and centimeter data and present a
review of the outflows and Herbig-Haro objects so far discovered in these
clouds.
