Table 5: Hot component of FN Sgr.
JD¹/phase Temperature Luminosity $^2~~[L_{\odot}]$

$\chi_{\rm max}$ [eV] $T_{\rm el}$ [10³ K] $L_{\rm h}(\rm H\beta)$ $L_{\rm h}(He {\sc ii}4686)$ $L_{\rm h}\rm (UV)$ $L_{\rm h}$ (A-F)

48 117/0.212³ 114

48 190/0.360³ 114 170 1460 1800 1440

48 203/0.366³ 114 150 1080 1200 430

49 945/0.428 114 150 1200 1500 1200 540

50 590/0.563 55 70 1530 1500 1080 1940

51 065-70/0.402 55 58: 1420 945: 1000 1940

51 325/0.856 55 127 1030 1240 1080 970

51 755-7/0.614 100 160 1420 1800 1440 1400

51 791/0.686 100 180 1900 2700 2200 1620

51 826-8/0.738 114 150 1850 2400 1800 540

52 133-5/0.279 114 170 1170 1550 1200 430

¹ Julian Date = 2 400 000 + JD listed in table; ² assumes d=7.5 kpc and E_B-V=0.2;
³ Based on emission line fluxes from Barbá et al. (1992).

**Table 5:** Hot component of FN Sgr.
JD¹/phase	Temperature	Luminosity $^2~~[L_{\odot}]$
	$\chi_{\rm max}$ [eV]	$T_{\rm el}$ [10³ K]	$L_{\rm h}(\rm H\beta)$	$L_{\rm h}(He {\sc ii}4686)$	$L_{\rm h}\rm (UV)$	$L_{\rm h}$ (A-F)
48 117/0.212³	114
48 190/0.360³	114	170	1460	1800	1440
48 203/0.366³	114	150	1080	1200	430
49 945/0.428	114	150	1200	1500	1200	540
50 590/0.563	55	70	1530	1500	1080	1940
51 065-70/0.402	55	58:	1420	945:	1000	1940
51 325/0.856	55	127	1030	1240	1080	970
51 755-7/0.614	100	160	1420	1800	1440	1400
51 791/0.686	100	180	1900	2700	2200	1620
51 826-8/0.738	114	150	1850	2400	1800	540
52 133-5/0.279	114	170	1170	1550	1200	430

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations
	3 Analysis and discussion
	4 Reddening and distance
	5 The nebula
	6 Hot component
	7 Conclusions
	References
	Online Material