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Table 1:

List of analyzed PNe.

PN G 		Name Pop. Ref. IR spectra
        PAH SiO cr. SiO am.
DC$_{\rm cr}$:            

000.1+04.3 		H 1-16 b P + + -
007.2+01.8 Hb 6 d P + + -
354.2+04.3 M 2-10 b G + + -
358.7-05.2 H 1-50 b P + + -

358.9+03.2 		H 1-20 b G + + -
DC $_{\rm a+cr}$:            

354.5+03.3 		Th 3-4 b P + + +
356.9+04.4 M 3-38 b P + + +
358.2+04.2 M 3-8 b P + + +

359.7-02.6 		H 1-40 b P + + +
OC $_{\rm a+cr}$:            

002.2-02.7 		M 2-23 b P - + +
008.2+06.8 He 2-260 d P - + +
355.6-02.7 H 1-32 b P - + +
355.7-03.5 H 1-35 b P - + +

Notes. The Galactic bulge (b) or disk (d) association of the object is marked in Col. 3. The reference to original observers is given in Col. 4. Objects are divided into three groups according to their infrared properties as marked in Cols. 5-7 (see description in Sect. 3).

References. G - Gutenkunst et al. (2008); P - Perea-Calderón et al. (2009).


Source LaTeX | All tables | In the text

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