Table 7: $T_{\star }$ and $L_{\star }$ of the PNe in Sextans A and Sextans B as derived with the modelling with CLOUDY.
Galaxy Name $T_{\star }$ (K) $\log~$ ( $L_{\star }$ / $L_{\odot}$ )

Sextans A PN 194 000 3.9

Sextans B PN1 61 000 3.5

PN2 78 000 3.3

PN3 72 000 3.5

PN4 65 000 3.2

PN5 90 000 3.6

**Table 7:** $T_{\star }$ and $L_{\star }$ of the PNe in Sextans A and Sextans B as derived with the modelling with CLOUDY.
Galaxy	Name	$T_{\star }$ (K)	$\log~$ ( $L_{\star }$ / $L_{\odot}$ )
Sextans A	PN	194 000	3.9
Sextans B	PN1	61 000	3.5
	PN2	78 000	3.3
	PN3	72 000	3.5
	PN4	65 000	3.2
	PN5	90 000	3.6

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and data reduction
	3 Chemical abundances of planetary nebulae and H II regions
	4 The peculiar PN of Sextans A
	5 Summary
	References