Free Access
Issue
A&A
Volume 578, June 2015
Article Number A132
Number of page(s) 37
Section Astrophysical processes
DOI https://doi.org/10.1051/0004-6361/201425167
Published online 16 June 2015

Online material

Table 1

Key parameters and mass fractions of nuclides (selected from the top 50 species) produced in collapsar accretions for cases A1-3 and B1-3.

Table 2

Final mass fractions of explosive nucleosynthesis in the outflows associated with GRBs at r = 3rsch for cases A1-3 and B1-3.

Table 3

As Table 2, but for cases A1-3 and B1-3 at r = 10rsch.

Table 4

As Table 2, but for cases A1-3 and B1-3 at r = 20rsch.

Table 5

As Table 2, but for cases A1-3 and B1-3 at r = 30rsch.

Table 6

As Table 2, but for cases A1-3 and B1-3 at r = 40rsch.

Table 7

As Table 2, but for cases A1-3 and B1-3 at r = 50rsch.

Table 8

Total yields after radioactive decays in the final step tf for 1 M matter ejected from outflows associated with GRBs.

thumbnail Fig. 3

Explosive nucleosynthesis in the outflow region associated with GRB for case A1 at r = 3rsch (case A1r = 3). The radioactive decays have been taken into account within the dynamic process [ t0,tf), but did not include the final step (tf), which can prevent some decayed species, as shown in this picture, from precipitously dropping to zero in the final step tf.

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thumbnail Fig. 4

As Fig. 3, but for case A1 at r = 50rsch (case A1r = 50). It only shows the long (relative) half-life species (τ0.5> 1 day) by considering the timing of observations; the species with half-lives of τ0.5 1 day are not plotted. The final abundances of nuclides as shown in this figure (selected from Table 7) exceed 10-11.

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thumbnail Fig. 5

Five up-species abundance increase when the value of collapsar accretion rate increases in panels a)c) in the left column and in panels d)f) in the right column. The other five down-species abundances decrease as increases. The abscissa is scaled in the value of . In a same panel, the same colors denote the same chemical species.

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© ESO, 2015

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