Table 3: Properties of the 1.5 $M_\odot$ model at the moments the structure plots of Fig. 10 were made. The age is in Gyr, the helium and carbon-oxygen core masses in $M_\odot$ . The last two columns give the mass fraction ratio Ne/O in the core, and the ratio of this number to the initial (ZAMS or ISM) Ne/O ratio.
Model Age $M_{\rm He}$ $M_{\rm CO}$ (Ne/O) $_{\rm c}$ (Ne/O) $_{\rm c}$ /(Ne/O) $_{\rm in}$

TAMS 2.5949 0.166 0.000 1.093 5.97

RGB 2.8495 0.440 0.000 1.093 5.97

AGB 2.9852 0.568 0.379 0.0260 0.142

**Table 3:** Properties of the 1.5 $M_\odot$ model at the moments the structure plots of Fig. 10 were made. The age is in Gyr, the helium and carbon-oxygen core masses in $M_\odot$ . The last two columns give the mass fraction ratio Ne/O in the core, and the ratio of this number to the initial (ZAMS or ISM) Ne/O ratio.
Model	Age	$M_{\rm He}$	$M_{\rm CO}$	(Ne/O) $_{\rm c}$	(Ne/O) $_{\rm c}$ /(Ne/O) $_{\rm in}$
TAMS	2.5949	0.166	0.000	1.093	5.97
RGB	2.8495	0.440	0.000	1.093	5.97
AGB	2.9852	0.568	0.379	0.0260	0.142

Source LaTeX | All tables | In the text

	1 Introduction
	2 Synopsis of X-ray bursts from 2S 0918-549
	3 Analysis of the long burst
	4 Flux history of persistent emission
	5 Discussion
	6 Conclusion
	References