Can massive Be/Oe stars be progenitors of long gamma ray bursts?

Free Access

Table 3:

Ratios of the ZAMS $\Omega /\Omega _{\rm {c}}$ per mass category of SMC Oe/Be stars corrected for the effect of magnetic field from the comparison between Ekström et al. (2008b) and Yoon et al. (2006) models.
Mass category	$\Omega /\Omega _{\rm {c}}$	$\Omega /\Omega _{\rm {c}}$ $-\sigma$	$\Omega /\Omega _{\rm {c}}$ $+\sigma$
A	0.77	0.69	0.88
A $-\sigma$ M	0.82	0.72	0.90
A $+\sigma$ M	0.74	0.65	0.83
B	0.76	0.59	0.94
B $-\sigma$ M	0.81	0.63	0.99
B $+\sigma$ M	0.71	0.56	0.88
C	0.80	0.62	0.94
C $-\sigma$ M	0.82	0.62	0.95
C $+\sigma$ M	0.79	0.61	0.92
D	0.79	0.55	0.93
D $-\sigma$ M	0.82	0.57	0.98
D $+\sigma$ M	0.76	0.52	0.89
E	0.83	0.70	0.92
E $-\sigma$ M	0.93	0.79	1.03
E $+\sigma$ M	0.75	0.63	0.82

Notes. Boldfaced values correspond to the average $\Omega /\Omega _{\rm {c}}$ ratios of subsamples.

Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.