Sixteen planetary nebulae and a shocked peculiar nebula were discovered in
the direction of the Galactic Center by means of direct inspection of the P
alomar Observatory and ESO/SERC sky surveys. For all objects we obtained na
rrow band H alpha imaging and medium resolution spectroscopy, allowing us t
o derive the basic parameters of the emission nebulae. For half of the nebu
lae of the sample, the central star candidate was identified and an estimat
e of the star temperature and luminosity is given.