TY - GEN
T1 - Galactic chemical evolution and 26 Al production by supernovae
AU - Timmes, F. X.
AU - Woosley, S. E.
AU - Weaver, Thomas A.
N1 - Publisher Copyright:
© 1993 American Institute of Physics.
PY - 1993
Y1 - 1993
N2 - Nucleosynthesis in the intermediate mass range (carbon through nickel) has been calculated for a grid of stellar masses between 10 and 40 M ⊙ for solar metallicity, and 12 and 75 M ⊙ for zero metallicity, with a total of 26 stars evolved to the presupernova state. Explosions have been simulated in 13 of these and the final nucleosynthetic yields, including the ν-process, determined. Except for the products of the neutrino process (fluorine and boron), the presupernova abundances of isotopes lighter than about A = 40 (including 26 Al), closely resemble the final yields. These results, when incorporated into a multi-zone model for Galactic chemical evolution that includes contributions from lower mass stars and Type Ia supernovae, give present day abundances that are in good agreement with those observed in the solar system when a particular choice is made for the 12 C (α ,γ) 16 Oreaction rate (S(300 keV) = 0.17 MeV barns). We find the production rate of "Al in the present epoch to be 1.78 - 2.14 M ⊙ Myr -1 , depending on the choice and range of the initial mass function. This result, which is consistent with the HEAO-3, SMM, and so far the Comptel observations, suggests that the dominant source of 26 Al in the Galaxy is from the supernova of Types II and Ib.
AB - Nucleosynthesis in the intermediate mass range (carbon through nickel) has been calculated for a grid of stellar masses between 10 and 40 M ⊙ for solar metallicity, and 12 and 75 M ⊙ for zero metallicity, with a total of 26 stars evolved to the presupernova state. Explosions have been simulated in 13 of these and the final nucleosynthetic yields, including the ν-process, determined. Except for the products of the neutrino process (fluorine and boron), the presupernova abundances of isotopes lighter than about A = 40 (including 26 Al), closely resemble the final yields. These results, when incorporated into a multi-zone model for Galactic chemical evolution that includes contributions from lower mass stars and Type Ia supernovae, give present day abundances that are in good agreement with those observed in the solar system when a particular choice is made for the 12 C (α ,γ) 16 Oreaction rate (S(300 keV) = 0.17 MeV barns). We find the production rate of "Al in the present epoch to be 1.78 - 2.14 M ⊙ Myr -1 , depending on the choice and range of the initial mass function. This result, which is consistent with the HEAO-3, SMM, and so far the Comptel observations, suggests that the dominant source of 26 Al in the Galaxy is from the supernova of Types II and Ib.
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U2 - 10.1063/1.44247
DO - 10.1063/1.44247
M3 - Conference contribution
AN - SCOPUS:85063824859
T3 - AIP Conference Proceedings
SP - 64
EP - 69
BT - Compton Gamma-Ray Observatory
A2 - Gehrels, Neil
A2 - Friedlander, Michael W.
A2 - Macomb, Daryl J.
PB - American Institute of Physics Inc.
T2 - Compton Symposium
Y2 - 15 October 1992 through 17 October 1992
ER -