Supernova progenitor stars in the initial range of 23 to 33 solar masses and their relation with the SNR Cassiopeia A

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Table 3:

Final stellar models.
Model	$M_{\rm f}$	M(He)	M(CO)	$M_{\rm env}$	$R_{\rm fin}/R_\odot$	$T_{\rm eff} \rm (K)$
23	13.2	6.45	2.23	6.75	700	4111
28	9.36	8.97	3.37	0.29	100	11 688
29	9.95	9.31	3.07	0.34	270	7509
30	5.85	5.85	2.86	-	3	57 430
33	4.57	4.57	2.93	-	36	15 719

Note: $M_{\rm f}$ refers to final stellar mass, M(He) is He-core mass, M(CO) is CO core, $M_{\rm env}$ is the stellar envelope mass and $R_{\rm fin}/R_\odot$ is the final stellar radius. All masses are shown in the units of $M_{\odot }$ .

Source LaTeX | All tables | In the text

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