  We present 21-cm HI line and optical R-band observations for a sample of 26
edge-on galaxies. The HI observations were obtained with the Westerbork
Synthesis Radio Telescope, and are part of the WHISP database (Westerbork HI
Survey of Spiral and Irregular Galaxies). We present HI maps, optical images,
and radial HI density profiles. We have also derived the rotation curves and
studied the warping and lopsidedness of the HI disks.
  20 out of the 26 galaxies of our sample are warped, confirming that warping
of the HI disks is a very common phenomenon in disk galaxies. Indeed, we find
that all galaxies that have an extended HI disk with respect to the optical are
warped.
  The warping usually starts around the edge of the optical disk. The degree of
warping varies considerably from galaxy to galaxy. Furthermore, many warps are
asymmetric, as they show up in only one side of the disk or exhibit large
differences in amplitude in the approaching and receding sides of the galaxy.
These asymmetries are more pronounced in rich environments, which may indicate
that tidal interactions are a source of warp asymmetry. A rich environment
tends to produce larger warps as well. The presence of lopsidedness seems to be
related to the presence of nearby companions.
