Abstract
The observational study of GLMP 621 have identified it as a newly-formed planetary nebula. In order to observe the system in more detail we have obtained images of this source, reported here, using the 2.5 m NOT Telescope with the ALFOSC camera together with a set of narrow band filters (see Riera et al. 2003). High-dispersion spectroscopic observations were also obtained. The complex geometry and kinematics observed in GLMP 621 resembles that of other Proto-PNe with a multipolar structure within a spherical halo.
