3 Results

The results are presented in Figs. 1 to 33. A few comments where appropriate have been given below. Note that each image has a size bar superimposed on it, to make scaling of the objects easy. The size of the bars varies but in all cases the projected length is 20$^{\prime\prime}$. For many objects with a wide dynamical range of emission we plot their images with a double grey scale to show better the details of the bright region. In all cases north is up, and east is to the left.

In Table 2 we list the observed objects. We give: index number, RA and Dec (2000.0), Galactic coordinate name, corresponding Figure No., image sizes and seeing FWHM on the same frame for all filters taken.

In Table 3 we give an alphabetical list of object names to make searching for a given PN easier.

Comments on Table 2:

1.

The H$\beta$ image probably has been taken through an H$\alpha$filter by mistake, hence the strong similarity between the two images presented.

2.

Possible planetary nebulae according to Acker et al. (1992).

  

Table 2: List of observed objects. For each image PN size (in arcsec), exposure time (in minutes), and seeing (in arcsec) are given. Images not taken with the Dutch Telescope are indicated with the superscripted letter b or c (see Table 1), and comments are indicated by numerical superscripts. All figures have north up, east to the left

 

Table 2: continued

  

Table 3: Alphabetical list of objects

Acknowledgements

S.K. Górny acknowledges the Nordic Optical Telescope Scientific Association for providing the opportunity to work on these data at La Palma and financial support from the grant No. 2.P03D.027.10 of the Polish Committee for Scientific Research.

 

Figure 1: M 1-28 (left), and M 3-2 (right)

 

Figure 2: He 2-67 (left), and NGC 3195 (right)

 

Figure 3: H 1-51 (top), He 2-70 (middle), and He 2-76 (bottom)

 

Figure 4: He 2-82 (top), He 2-84 (middle), and He 2-114 (bottom)

 

Figure 5: He 2-116 (top), He 2-119 (middle), and He 2-120 (bottom)

 

Figure 6: He 2-145 (top), He 2-146 (middle), and He 2-152 (bottom)

 

Figure 7: He 2-153 (top), He 2-155 (middle), and He 2-161 (bottom)

 

Figure 8: He 2-164 (top), He 2-165 (middle), and He 2-169 (bottom)

 

Figure 9: Hf 2-1 (top), Ic 4148-50 (middle), and M 1-151 (bottom)

 

Figure 10: M 3-51 (top), Mz 2 (middle), and NGC 2818 (bottom)

 

Figure 11: NGC 2899 (top), NGC 3699 (middle), and NGC 5189 (bottom)

 

Figure 12: Pe 1-8 (top), A 26 (middle left), A 7 (middle right), Anon. 19h19m (bottom left), Cn 1-1 (bottom right)

 

Figure 13: H 1-43 (top), Hb 7 (middle), and He 2-11 (bottom)

 

Figure 14: He 2-18 (top), He 2-28 (middle), and He 2-29 (bottom)

 

Figure 15: He 2-35 (top), He 2-37 (middle), and He 2-39 (bottom)

 

Figure 16: He 2-47 (top), He 2-63 (middle), and He 2-68 (bottom)

 

Figure 17: He 2-77 (top), He 2-78 (middle), and He 2-81 (bottom)

 

Figure 18: He 2-83 (top), He 2-85 (middle), and He 2-86 (bottom)

 

Figure 19: He 2-88 (top), He 2-96 (middle), and He 2-102 (bottom)

 

Figure 20: He 2-103 (top), He 2-109 (middle), and He 2-111 (bottom)

 

Figure 21: He 2-112 (top), He 2-115 (middle), and He 2-129 (bottom)

 

Figure 22: He 2-132 (top), He 2-138 (middle), and He 2-140 (bottom)

 

Figure 23: He 2-143 (top), He 2-147 (middle), and He 2-159 (bottom)

 

Figure 24: He 2-163 (top), He 2-207 (middle), and He 2-436 (bottom)

 

Figure 25: K 2-7 (top), Lo 12 (middle), and Lo 13 (bottom)

 

Figure 26: Lo 14 (top), M 1-13 (middle), and M 1-14 (bottom)

 

Figure 27: M 1-17 (top), M 1-47 (middle), and M 1-62 (bottom)

 

Figure 28: Me 2-19 (top), M 3-1 (middle), and M 3-29 (bottom)

 

Figure 29: M 3-32 (top), M 3-33 (middle), and M 3-39 (bottom)

 

Figure 30: Mz 3 (top & middle), and NGC 246 (bottom)

 

Figure 31: NGC 3211 (top), NGC 4071 (middle), and NGC 5307 (bottom)

 

Figure 32: NGC 6153 (top), PB 1 (middle), and Pe 1-3 (bottom)

  

Figure 33: Pe 1-6 (top), Pe 2-7 (middle), and Pe 2-8 (bottom)

 

Figure 34: Pe 2-14 (top), Ps 1 (middle), and TH 2-A (bottom)