New asymptotic giant branch models for a range of metallicities

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Volume 508 / No 3 (December IV 2009)

A&A, 508 3 (2009) 1343-1358

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Table C.1:

Post-AGB evolution for all models with solar-scaled metal distributions computed through this phase^a.
$M_{{\rm ZAMS}}$	$T_{{\rm eff,i}}$	$M_{{\rm T4}}$	$t_{\rm tr}$	$t_{\rm 1}$	$t_{\rm cr}$	?-burner	TP	End
Z = 0.0005 / solar
1.0	3.68	0.537	4.274	5.365	14.464	H	no	WD
1.2	3.69	0.550	2.403	2.868	8.845	H	no	WD
1.5	3.72	0.579	0.905	1.008	3.441	H	no	WD
1.6	3.72	0.578	1.076	1.213	4.129	H	no	WD
1.8	3.71	0.565	0.545	0.860	3.917	H	no	WD
2.0	3.73	0.600	0.335	0.478	2.412	H	no	WD
Z = 0.004 / solar
1.0	3.71*	0.528	0.030	1.116*	16.348	H	no	WD
1.2	3.71*	0.531	0.032	1.386*	16.816	H	no	W
1.5	3.71*	0.536	0.276	0.681*	8.149	H/He	VLTP	2 $^{\rm nd}$ AGB
1.6	3.69	0.536	1.605	1.909	6.330	H	no	WD
1.8	3.71*	0.492	0.020	1.029*	2.810	H/He	LTP	2 $^{\rm nd}$ AGB
2.0	3.68	0.528	1.325	2.770	10.709	H	no	WD
Z = 0.008 / solar
1.0	3.70*	0.531	0.577	1.730*	16.935	H/He	VLTP	2 $^{\rm nd}$ AGB
1.2	3.71*	0.529	0.027	0.030*	14.369	H	no	WD
1.5	3.69	0.537	1.840	2.178	6.995	H/He	VLTP	during VLTP
1.6	3.72*	0.537	0.192	0.443*	5.595	H/He	VLTP	2 $^{\rm nd}$ AGB
1.8	3.72*	0.526	0.021	0.025*	12.811	H	no	WD
2.0	3.73*	0.528	0.013	0.014*	5.173	H	no	WD
Z = 0.02 / solar
1.0	3.71*	0.506	0.037	0.041*	26.417	H	no	WD
1.2	3.70*	0.523	0.033	0.038*	16.099	H	no	WD
1.5	3.70*	0.538	0.445	0.832*	7.388	H	no	WD
1.6	3.72*	0.541	0.020	0.021*	6.248	H/He	VLTP	2 $^{\rm nd}$ AGB
1.8	3.73*	0.524	0.667	29.316*	47.833	H	no	WD
2.0	3.70	0.543	0.528	0.868	3.614	H	no	WD
Z = 0.04 / solar
1.0	3.57	49.717	0.510	57.677	86.516	He	no	WD
1.2	3.60	4.042	0.522	31.515	48.850	He	no	WD
1.5	3.64	7.858	0.531	10.215	18.553	H	no	WD
1.6	3.71*	0.021	0.536	0.029*	6.926	H	no	WD
1.8	3.70*	0.783	0.536	1.805*	6.875	H	no	WD
2.0	3.70	0.628	0.552	1.131	4.523	H	no	WD

^a See text for explanation of column contents; all times in 10³ years.

Source LaTeX | All tables | In the text

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