Table 6: Main characteristics derived from the optical images and spectra of the IRAS sources identified as PNe.
IRAS name PN G name Other names Morphology Size ( $^{\prime\prime}$) c Excitation class WR subtype Code$^\dagger$
06518-1041 222.8-04.2 PM 1-23 Bipolar 20 1.1   [WC7] AA
07027-7934 291.3-26.2   Round <15 2.3   [WC10] AA
08046-3844 255.3-03.6   Compact - 1.5 Medium   AA
08355-4027 260.7+00.9 PM 1-41 Round 12 3.0 Medium   AA
08418-4843     - - 2.5 Medium   AA
08574-5011 270.1-02.9   Round 10 2.7 Medium   AA
09362-5413 277.1-01.5   Compact <2 2.8 Low   AA
09517-5438 279.1-00.4   - - 2.4 Medium   AA
10029-5553 281.1-00.4 PM 2-10 Compact <3.4 High -   AB
10115-5640 282.6-00.4 PM 1-51 Compact <6.1 High -   AB
12316-6401 301.1-01.4 PM 1-68 Compact <2.3 1.1 Medium   AA
14079-6402     Compact - 2.2 Low   AA
14122-5947 313.3+01.1   Elliptical/Bipolar <4.5 High -   AA
14177-5824 314.4+02.2 PM 1-81 Bipolar 6 4.9 Medium   AA
14345-5858 316.2+00.8   - <9.9 High -   AA
15154-5258 324.0+03.5 PM 1-89 Round 10 0.9   [WC4] AA
15559-5546 327.1-02.2 Hen 2-142 Elliptical/Bipolar 5.3$\times$3.2 1.4   [WC9] AA
15579-5445 328.0-01.6 PM 1-105 - <1.8 High -   AA
16053-5528 328.4-02.8 PM 1-106 - - 2.8 Low   AA
16114-4504 336.1+04.1 PM 2-17 Elliptical? 8 3.0 High   AA
16529-4341 342.2-00.3 PM 1-119 - <4.7 High -   AA
17088-4227 344.9-01.9 PM 1-131 - <2.2 High -   AA
17119-5926 331.3-12.1 Hen 3-1357 Elliptical/Bipolar $2.1\times1.9$ 0.3 Medium   AA
17131-3330   PM 1-136 RPZM 10 - <1.6 High -   AA
17164-3226   PM 1-140 RPZM 12 - <2.1 2.84 Medium   CA
17371-2747   OH6 - - 4.7 Low   AA
17381-1616 010.2+07.5 PM 2-28 - - High -   AA
17395-0841 017.0+11.1   Bipolar $5\times8$ 1.9 Low   AA
17514-1555 012.2+04.9 PM 1-188 Round 18 1.2   [WC9] AA
17597-1442 014.2+03.8 PM 1-205 Round 20 0.8   [WC9] AA
18061-2505 005.9-02.6 PM 1-213 Bipolar $15\times46$ 2.1 Low   AA
18186-0833 021.9+02.7 PM 1-226 Round 8 2.31 Medium   AA
18401-1109 022.0-03.1 PM 1-252 Elliptical $9\times11$ 1.0 High   AA
18520+0007     Compact - High -   AB
19154+0809 043.2-02.0 PM 2-40 Compact - 2.7 Low   AA
19589+3419 070.9+02.2 PM 1-316 Compact? - - Low   AA
$\dagger$ This code rates our confidence in the data presented, with A representing the maximum reliability. The first letter marks our confidence in the correct identification of the optical counterpart, and the second letter indicates how confident we are in the evolutionary classification assigned.

* Spectroscopic range covered not enough to assign a classification.


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