Nucleosynthetic yields of stable isotopes for all cases after the simulation. The first column for each q gives the ratio of the final abundance to the solar value, the second column gives the mass fraction of each species still bound to the WD, and the third column gives mass fraction of each still unbound with respect to the WD. The amount of MS star material bound to the WD is 0.16, 0.35, and 0.94 |${\rm M}_{\odot }$| for |$q=0.5, 1,\ \mathrm{ and} \ 2$|, respectively.
| . | q = 0.5 . | q = 1 . | q = 2 . | ||||||
|---|---|---|---|---|---|---|---|---|---|
| Species . | Final/solar . | Bound . | Unbound . | Final/solar . | Bound . | Unbound . | Final/solar . | Bound . | Unbound . |
| |$^{1}$|H | 0.997 | 0.706 | 0.707 | 0.998 | 0.707 | 0.707 | 0.998 | 0.707 | 0.707 |
| |$^{4}$|He | 0.999 | 0.276 | 0.276 | 0.998 | 0.276 | 0.276 | 0.998 | 0.276 | 0.276 |
| |$^{7}$|Li | 0.026 | |$1.66 \times 10^{-12}$| | |$5.25 \times 10^{-10}$| | 0.356 | |$2.17 \times 10^{-9}$| | |$5.01 \times 10^{-9}$| | 0.644 | |$6.11 \times 10^{-9}$| | |$5.85 \times 10^{-9}$| |
| |$^{7}$|Be|$^{*}$| | |$3.87 \times 10^{-6}$| | |$2.56 \times 10^{-6}$| | |$3.60 \times 10^{-7}$| | |$1.15 \times 10^{-6}$| | |$1.04 \times 10^{-6}$| | |$1.31 \times 10^{-6}$| | |$3.94 \times 10^{-7}$| | |$2.85 \times 10^{-7}$| | |$7.29 \times 10^{-7}$| |
| |$^{8}$|B|$^{*}$| | |$1.19 \times 10^{-9}$| | |$4.47 \times 10^{-10}$| | |$6.29 \times 10^{-11}$| | |$6.91 \times 10^{-10}$| | |$1.17 \times 10^{-9}$| | |$1.35 \times 10^{-15}$| | |$2.15 \times 10^{-10}$| | |$2.85 \times 10^{-10}$| | |$5.30 \times 10^{-13}$| |
| |$^{12}$|C | 0.722 | |$1.94 \times 10^{-3}$| | |$2.49 \times 10^{-3}$| | 0.911 | |$2.73 \times 10^{-3}$| | |$2.82 \times 10^{-3}$| | 0.977 | |$2.99 \times 10^{-3}$| | |$2.93 \times 10^{-3}$| |
| |$^{13}$|C | 3.686 | |$2.13 \times 10^{-4}$| | |$4.70 \times 10^{-5}$| | 2.247 | |$1.03 \times 10^{-4}$| | |$1.18 \times 10^{-5}$| | 1.352 | |$4.81 \times 10^{-5}$| | |$5.40 \times 10^{-5}$| |
| |$^{14}$|N | 1.382 | |$1.80 \times 10^{-3}$| | |$1.23 \times 10^{-3}$| | 1.110 | |$1.27\times 10^{-3}$| | |$1.18 \times 10^{-3}$| | 1.023 | |$1.13 \times 10^{-3}$| | |$1.14 \times 10^{-3}$| |
| |$^{15}$|N | 80.01 | |$4.93 \times 10^{-4}$| | |$1.89 \times 10^{-4}$| | 17.02 | |$7.33 \times 10^{-5}$| | |$7.64 \times 10^{-5}$| | 5.309 | |$1.89 \times 10^{-5}$| | |$3.65 \times 10^{-5}$| |
| |$^{16}$|O | 0.819 | |$7.36 \times 10^{-3}$| | |$8.49 \times 10^{-3}$| | 0.964 | |$9.25 \times 10^{-3}$| | |$9.33 \times 10^{-3}$| | 0.992 | |$9.56 \times 10^{-3}$| | |$9.52 \times 10^{-3}$| |
| |$^{17}$|O | 171.1 | |$9.41 \times 10^{-4}$| | |$3.59 \times 10^{-4}$| | 39.52 | |$1.63 \times 10^{-4}$| | |$1.42 \times 10^{-4}$| | 8.267 | |$2.80 \times 10^{-5}$| | |$4.51 \times 10^{-5}$| |
| |$^{18}$|O | 0.541 | |$9.30 \times 10^{-6}$| | |$1.46 \times 10^{-5}$| | 0.820 | |$1.72 \times 10^{-5}$| | |$1.87 \times 10^{-5}$| | 0.948 | |$2.10 \times 10^{-5}$| | |$1.95 \times 10^{-6}$| |
| |$^{19}$|F | 0.658 | |$2.08 \times 10^{-7}$| | |$3.35 \times 10^{-7}$| | 0.903 | |$3.61 \times 10^{-7}$| | |$3.76 \times 10^{-7}$| | 0.976 | |$3.98 \times 10^{-7}$| | |$3.93 \times 10^{-7}$| |
| |$^{20}$|Ne | 0.945 | |$1.54 \times 10^{-3}$| | |$1.54 \times 10^{-3}$| | 0.992 | |$1.61 \times 10^{-3}$| | |$1.61 \times 10^{-3}$| | 0.997 | |$1.62 \times 10^{-3}$| | |$1.62 \times 10^{-3}$| |
| . | q = 0.5 . | q = 1 . | q = 2 . | ||||||
|---|---|---|---|---|---|---|---|---|---|
| Species . | Final/solar . | Bound . | Unbound . | Final/solar . | Bound . | Unbound . | Final/solar . | Bound . | Unbound . |
| |$^{1}$|H | 0.997 | 0.706 | 0.707 | 0.998 | 0.707 | 0.707 | 0.998 | 0.707 | 0.707 |
| |$^{4}$|He | 0.999 | 0.276 | 0.276 | 0.998 | 0.276 | 0.276 | 0.998 | 0.276 | 0.276 |
| |$^{7}$|Li | 0.026 | |$1.66 \times 10^{-12}$| | |$5.25 \times 10^{-10}$| | 0.356 | |$2.17 \times 10^{-9}$| | |$5.01 \times 10^{-9}$| | 0.644 | |$6.11 \times 10^{-9}$| | |$5.85 \times 10^{-9}$| |
| |$^{7}$|Be|$^{*}$| | |$3.87 \times 10^{-6}$| | |$2.56 \times 10^{-6}$| | |$3.60 \times 10^{-7}$| | |$1.15 \times 10^{-6}$| | |$1.04 \times 10^{-6}$| | |$1.31 \times 10^{-6}$| | |$3.94 \times 10^{-7}$| | |$2.85 \times 10^{-7}$| | |$7.29 \times 10^{-7}$| |
| |$^{8}$|B|$^{*}$| | |$1.19 \times 10^{-9}$| | |$4.47 \times 10^{-10}$| | |$6.29 \times 10^{-11}$| | |$6.91 \times 10^{-10}$| | |$1.17 \times 10^{-9}$| | |$1.35 \times 10^{-15}$| | |$2.15 \times 10^{-10}$| | |$2.85 \times 10^{-10}$| | |$5.30 \times 10^{-13}$| |
| |$^{12}$|C | 0.722 | |$1.94 \times 10^{-3}$| | |$2.49 \times 10^{-3}$| | 0.911 | |$2.73 \times 10^{-3}$| | |$2.82 \times 10^{-3}$| | 0.977 | |$2.99 \times 10^{-3}$| | |$2.93 \times 10^{-3}$| |
| |$^{13}$|C | 3.686 | |$2.13 \times 10^{-4}$| | |$4.70 \times 10^{-5}$| | 2.247 | |$1.03 \times 10^{-4}$| | |$1.18 \times 10^{-5}$| | 1.352 | |$4.81 \times 10^{-5}$| | |$5.40 \times 10^{-5}$| |
| |$^{14}$|N | 1.382 | |$1.80 \times 10^{-3}$| | |$1.23 \times 10^{-3}$| | 1.110 | |$1.27\times 10^{-3}$| | |$1.18 \times 10^{-3}$| | 1.023 | |$1.13 \times 10^{-3}$| | |$1.14 \times 10^{-3}$| |
| |$^{15}$|N | 80.01 | |$4.93 \times 10^{-4}$| | |$1.89 \times 10^{-4}$| | 17.02 | |$7.33 \times 10^{-5}$| | |$7.64 \times 10^{-5}$| | 5.309 | |$1.89 \times 10^{-5}$| | |$3.65 \times 10^{-5}$| |
| |$^{16}$|O | 0.819 | |$7.36 \times 10^{-3}$| | |$8.49 \times 10^{-3}$| | 0.964 | |$9.25 \times 10^{-3}$| | |$9.33 \times 10^{-3}$| | 0.992 | |$9.56 \times 10^{-3}$| | |$9.52 \times 10^{-3}$| |
| |$^{17}$|O | 171.1 | |$9.41 \times 10^{-4}$| | |$3.59 \times 10^{-4}$| | 39.52 | |$1.63 \times 10^{-4}$| | |$1.42 \times 10^{-4}$| | 8.267 | |$2.80 \times 10^{-5}$| | |$4.51 \times 10^{-5}$| |
| |$^{18}$|O | 0.541 | |$9.30 \times 10^{-6}$| | |$1.46 \times 10^{-5}$| | 0.820 | |$1.72 \times 10^{-5}$| | |$1.87 \times 10^{-5}$| | 0.948 | |$2.10 \times 10^{-5}$| | |$1.95 \times 10^{-6}$| |
| |$^{19}$|F | 0.658 | |$2.08 \times 10^{-7}$| | |$3.35 \times 10^{-7}$| | 0.903 | |$3.61 \times 10^{-7}$| | |$3.76 \times 10^{-7}$| | 0.976 | |$3.98 \times 10^{-7}$| | |$3.93 \times 10^{-7}$| |
| |$^{20}$|Ne | 0.945 | |$1.54 \times 10^{-3}$| | |$1.54 \times 10^{-3}$| | 0.992 | |$1.61 \times 10^{-3}$| | |$1.61 \times 10^{-3}$| | 0.997 | |$1.62 \times 10^{-3}$| | |$1.62 \times 10^{-3}$| |
Note. |$^{*}$|These isotopes show the final mass fraction and not the ratio to solar abundance in the first column of each q.
Nucleosynthetic yields of stable isotopes for all cases after the simulation. The first column for each q gives the ratio of the final abundance to the solar value, the second column gives the mass fraction of each species still bound to the WD, and the third column gives mass fraction of each still unbound with respect to the WD. The amount of MS star material bound to the WD is 0.16, 0.35, and 0.94 |${\rm M}_{\odot }$| for |$q=0.5, 1,\ \mathrm{ and} \ 2$|, respectively.
| . | q = 0.5 . | q = 1 . | q = 2 . | ||||||
|---|---|---|---|---|---|---|---|---|---|
| Species . | Final/solar . | Bound . | Unbound . | Final/solar . | Bound . | Unbound . | Final/solar . | Bound . | Unbound . |
| |$^{1}$|H | 0.997 | 0.706 | 0.707 | 0.998 | 0.707 | 0.707 | 0.998 | 0.707 | 0.707 |
| |$^{4}$|He | 0.999 | 0.276 | 0.276 | 0.998 | 0.276 | 0.276 | 0.998 | 0.276 | 0.276 |
| |$^{7}$|Li | 0.026 | |$1.66 \times 10^{-12}$| | |$5.25 \times 10^{-10}$| | 0.356 | |$2.17 \times 10^{-9}$| | |$5.01 \times 10^{-9}$| | 0.644 | |$6.11 \times 10^{-9}$| | |$5.85 \times 10^{-9}$| |
| |$^{7}$|Be|$^{*}$| | |$3.87 \times 10^{-6}$| | |$2.56 \times 10^{-6}$| | |$3.60 \times 10^{-7}$| | |$1.15 \times 10^{-6}$| | |$1.04 \times 10^{-6}$| | |$1.31 \times 10^{-6}$| | |$3.94 \times 10^{-7}$| | |$2.85 \times 10^{-7}$| | |$7.29 \times 10^{-7}$| |
| |$^{8}$|B|$^{*}$| | |$1.19 \times 10^{-9}$| | |$4.47 \times 10^{-10}$| | |$6.29 \times 10^{-11}$| | |$6.91 \times 10^{-10}$| | |$1.17 \times 10^{-9}$| | |$1.35 \times 10^{-15}$| | |$2.15 \times 10^{-10}$| | |$2.85 \times 10^{-10}$| | |$5.30 \times 10^{-13}$| |
| |$^{12}$|C | 0.722 | |$1.94 \times 10^{-3}$| | |$2.49 \times 10^{-3}$| | 0.911 | |$2.73 \times 10^{-3}$| | |$2.82 \times 10^{-3}$| | 0.977 | |$2.99 \times 10^{-3}$| | |$2.93 \times 10^{-3}$| |
| |$^{13}$|C | 3.686 | |$2.13 \times 10^{-4}$| | |$4.70 \times 10^{-5}$| | 2.247 | |$1.03 \times 10^{-4}$| | |$1.18 \times 10^{-5}$| | 1.352 | |$4.81 \times 10^{-5}$| | |$5.40 \times 10^{-5}$| |
| |$^{14}$|N | 1.382 | |$1.80 \times 10^{-3}$| | |$1.23 \times 10^{-3}$| | 1.110 | |$1.27\times 10^{-3}$| | |$1.18 \times 10^{-3}$| | 1.023 | |$1.13 \times 10^{-3}$| | |$1.14 \times 10^{-3}$| |
| |$^{15}$|N | 80.01 | |$4.93 \times 10^{-4}$| | |$1.89 \times 10^{-4}$| | 17.02 | |$7.33 \times 10^{-5}$| | |$7.64 \times 10^{-5}$| | 5.309 | |$1.89 \times 10^{-5}$| | |$3.65 \times 10^{-5}$| |
| |$^{16}$|O | 0.819 | |$7.36 \times 10^{-3}$| | |$8.49 \times 10^{-3}$| | 0.964 | |$9.25 \times 10^{-3}$| | |$9.33 \times 10^{-3}$| | 0.992 | |$9.56 \times 10^{-3}$| | |$9.52 \times 10^{-3}$| |
| |$^{17}$|O | 171.1 | |$9.41 \times 10^{-4}$| | |$3.59 \times 10^{-4}$| | 39.52 | |$1.63 \times 10^{-4}$| | |$1.42 \times 10^{-4}$| | 8.267 | |$2.80 \times 10^{-5}$| | |$4.51 \times 10^{-5}$| |
| |$^{18}$|O | 0.541 | |$9.30 \times 10^{-6}$| | |$1.46 \times 10^{-5}$| | 0.820 | |$1.72 \times 10^{-5}$| | |$1.87 \times 10^{-5}$| | 0.948 | |$2.10 \times 10^{-5}$| | |$1.95 \times 10^{-6}$| |
| |$^{19}$|F | 0.658 | |$2.08 \times 10^{-7}$| | |$3.35 \times 10^{-7}$| | 0.903 | |$3.61 \times 10^{-7}$| | |$3.76 \times 10^{-7}$| | 0.976 | |$3.98 \times 10^{-7}$| | |$3.93 \times 10^{-7}$| |
| |$^{20}$|Ne | 0.945 | |$1.54 \times 10^{-3}$| | |$1.54 \times 10^{-3}$| | 0.992 | |$1.61 \times 10^{-3}$| | |$1.61 \times 10^{-3}$| | 0.997 | |$1.62 \times 10^{-3}$| | |$1.62 \times 10^{-3}$| |
| . | q = 0.5 . | q = 1 . | q = 2 . | ||||||
|---|---|---|---|---|---|---|---|---|---|
| Species . | Final/solar . | Bound . | Unbound . | Final/solar . | Bound . | Unbound . | Final/solar . | Bound . | Unbound . |
| |$^{1}$|H | 0.997 | 0.706 | 0.707 | 0.998 | 0.707 | 0.707 | 0.998 | 0.707 | 0.707 |
| |$^{4}$|He | 0.999 | 0.276 | 0.276 | 0.998 | 0.276 | 0.276 | 0.998 | 0.276 | 0.276 |
| |$^{7}$|Li | 0.026 | |$1.66 \times 10^{-12}$| | |$5.25 \times 10^{-10}$| | 0.356 | |$2.17 \times 10^{-9}$| | |$5.01 \times 10^{-9}$| | 0.644 | |$6.11 \times 10^{-9}$| | |$5.85 \times 10^{-9}$| |
| |$^{7}$|Be|$^{*}$| | |$3.87 \times 10^{-6}$| | |$2.56 \times 10^{-6}$| | |$3.60 \times 10^{-7}$| | |$1.15 \times 10^{-6}$| | |$1.04 \times 10^{-6}$| | |$1.31 \times 10^{-6}$| | |$3.94 \times 10^{-7}$| | |$2.85 \times 10^{-7}$| | |$7.29 \times 10^{-7}$| |
| |$^{8}$|B|$^{*}$| | |$1.19 \times 10^{-9}$| | |$4.47 \times 10^{-10}$| | |$6.29 \times 10^{-11}$| | |$6.91 \times 10^{-10}$| | |$1.17 \times 10^{-9}$| | |$1.35 \times 10^{-15}$| | |$2.15 \times 10^{-10}$| | |$2.85 \times 10^{-10}$| | |$5.30 \times 10^{-13}$| |
| |$^{12}$|C | 0.722 | |$1.94 \times 10^{-3}$| | |$2.49 \times 10^{-3}$| | 0.911 | |$2.73 \times 10^{-3}$| | |$2.82 \times 10^{-3}$| | 0.977 | |$2.99 \times 10^{-3}$| | |$2.93 \times 10^{-3}$| |
| |$^{13}$|C | 3.686 | |$2.13 \times 10^{-4}$| | |$4.70 \times 10^{-5}$| | 2.247 | |$1.03 \times 10^{-4}$| | |$1.18 \times 10^{-5}$| | 1.352 | |$4.81 \times 10^{-5}$| | |$5.40 \times 10^{-5}$| |
| |$^{14}$|N | 1.382 | |$1.80 \times 10^{-3}$| | |$1.23 \times 10^{-3}$| | 1.110 | |$1.27\times 10^{-3}$| | |$1.18 \times 10^{-3}$| | 1.023 | |$1.13 \times 10^{-3}$| | |$1.14 \times 10^{-3}$| |
| |$^{15}$|N | 80.01 | |$4.93 \times 10^{-4}$| | |$1.89 \times 10^{-4}$| | 17.02 | |$7.33 \times 10^{-5}$| | |$7.64 \times 10^{-5}$| | 5.309 | |$1.89 \times 10^{-5}$| | |$3.65 \times 10^{-5}$| |
| |$^{16}$|O | 0.819 | |$7.36 \times 10^{-3}$| | |$8.49 \times 10^{-3}$| | 0.964 | |$9.25 \times 10^{-3}$| | |$9.33 \times 10^{-3}$| | 0.992 | |$9.56 \times 10^{-3}$| | |$9.52 \times 10^{-3}$| |
| |$^{17}$|O | 171.1 | |$9.41 \times 10^{-4}$| | |$3.59 \times 10^{-4}$| | 39.52 | |$1.63 \times 10^{-4}$| | |$1.42 \times 10^{-4}$| | 8.267 | |$2.80 \times 10^{-5}$| | |$4.51 \times 10^{-5}$| |
| |$^{18}$|O | 0.541 | |$9.30 \times 10^{-6}$| | |$1.46 \times 10^{-5}$| | 0.820 | |$1.72 \times 10^{-5}$| | |$1.87 \times 10^{-5}$| | 0.948 | |$2.10 \times 10^{-5}$| | |$1.95 \times 10^{-6}$| |
| |$^{19}$|F | 0.658 | |$2.08 \times 10^{-7}$| | |$3.35 \times 10^{-7}$| | 0.903 | |$3.61 \times 10^{-7}$| | |$3.76 \times 10^{-7}$| | 0.976 | |$3.98 \times 10^{-7}$| | |$3.93 \times 10^{-7}$| |
| |$^{20}$|Ne | 0.945 | |$1.54 \times 10^{-3}$| | |$1.54 \times 10^{-3}$| | 0.992 | |$1.61 \times 10^{-3}$| | |$1.61 \times 10^{-3}$| | 0.997 | |$1.62 \times 10^{-3}$| | |$1.62 \times 10^{-3}$| |
Note. |$^{*}$|These isotopes show the final mass fraction and not the ratio to solar abundance in the first column of each q.
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