The mixed chemistry phenomenon in Galactic Bulge PNe

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Volume 495 / No 2 (February IV 2009)

A&A, 495 2 (2009) L5-L8

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Table A.1:

The other Galactic Bulge PNe observed with Spitzer/IRS (program $\char93$ 3633).
IRAS name	PN name	RA	Dec	Spectral type^a	Optical diameter^e	Distance from GC	Dust type
		J2000.0	J2000.0		(arcsec)	( $\hbox{$^\circ$ }$ )
17230-3459	H 1-12	17 26 24.3	-35 01 41	unknown	6.8	7.33	O
17385-2211	M 3-13	17 41 36.6	-22 13 03	none^b	0.0	6.78	O
17427-3402	H 1-32	17 46 06.3	-34 03 45	none^b	<5.0	5.13	O
17459-3421	H 1-35	17 49 14.0	-34 22 52	none^c	2.0	5.50	O
17585-2825	M 2-23	18 01 42.7	-28 25 44	none^d	8.5	3.56	O

^a None - neither [WC] nor wels; ^b Górny et al. (2004); ^c Wang & Liu (2007); ^d Górny et al. (2008); ^e Strasbourg-ESO Catalogue of Galactic Planetary Nebulae Acker et al. (1992), 0.0 - PN is a point-like source.

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