Line energy | Nuclear | FWHMa | Fluxa |
(MeV) | Transition | (keV) | cm-2 s-1 |
0.718 | 10B
*0.718
![]() |
30 |
![]() |
0.847 | 56Fe
*0.847
![]() |
6 |
![]() |
27Al
*0.844
![]() |
|||
1.809 | 26Mg
*1.809
![]() |
<2.7c |
![]() |
(26Al decay) | |||
4.44 | 12C
*4.439
![]() |
160 |
![]() |
11B
*4.445
![]() |
|||
![]() |
14N
*5.106
![]() |
280 |
![]() |
15O
*5.181
![]() |
|||
15O
*5.241
![]() |
|||
15N
*5.270
![]() |
|||
15N
*5.299
![]() |
|||
![]() |
16O
*6.130
![]() |
180d |
![]() |
15O
*6.176
![]() |
|||
15N
*6.324
![]() |
a For
MeV nucleon-1 and
(see Eq. (4)). The fluxes are for the region of angular radius
(see
Fig. 3 for fluxes at 4.44 and
6.2 MeV calculated for lower values of
).
b Ground state.
c Assuming thermal broadening with T<10 keV.
d A very narrow line component at 6.129 MeV could arise from excitation
of 16O nuclei contained in micrometer-sized grains (see text).
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