In the vicinity of the southern hemisphere giant HII region NGC3603 we disc
overed a new planetary nebula: PN G291.4-00.3 located at RA(J2000.0) =11(h)
14(m) 32.(s)1 +/- 0.(s)3, DECJ2000.0 = 61 degrees 00'02 " +/- 100. Monochr
omatic images reveal a central ring-like structure accompanied by onsets of
arc-like filaments which might outline a bipolar out ow. Analysis of the n
ebula spectrum shows that helium and nitrogen are enriched, while oxygen, s
ulphur and argon abundances seem to be solar. The central star must be hot
(above 100 kK) and having a luminosity of more than 3000 L-circle dot. All
evidence shows that PN G291.4-00.3 is a high-excitation, density bounded pl
anetary nebula of the type I, coming from the high-mass end of the intermed
iate mass stars.