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Nucleosynthesis of CNO Isotopes

  • James W. Truran
Part of the Astrophysics and Space Science Library book series (ASSL, volume 67)

Abstract

The origin of the seven stable isotopes of carbon, nitrogen, and oxygen remains an unsolved problem. Current views as to the mechanisms of nucleosynthesis of these nuclei indicate a collective history which is extremely complex. Theoretical studies have revealed that quite varied astrophysical sites can contribute significantly to their production, including CNO-cycle hydrogen burning, core helium burning, thermal relaxation oscillations associated with double-shell-burning configurations in red giants, nova explosions, and supernova explosions. The relevance of detailed quantitative estimates of contributions from these diverse sites is clear from the discussions presented throughout this session: coupled to increasing observations of CNO elemental and isotopic abundances, such studies can yield important inferences concerning the history of the interstellar medium, the evolution of our galaxy and of other galaxies, the sources of cosmic rays, stellar evolution, and the mechanisms of nova and supernova explosions.

Keywords

Interstellar Medium Supernova Explosion Lower Mass Star Carbon Star Hydrogen Burning 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Appenzeller, I. and Fricke, K.: 1972, Astron. Astrophys. 21, 285.ADSGoogle Scholar
  2. Arnett, W. D.: 1972, Astrophys. J. 176, 681.ADSCrossRefGoogle Scholar
  3. Arnett, W. D. and Schramm, D. N.: 1973, Astrophys. J. Letters 185, L47.ADSCrossRefGoogle Scholar
  4. Audouze, J. and Fricke, K.: 1973, Astrophys. J. 186, 239.ADSCrossRefGoogle Scholar
  5. Audouze, J., Lequeux, J., and Vigroux, L.: 1975, Astron. Astrophys. 43, 71.ADSGoogle Scholar
  6. Audouze, J., Truran, J. W., and Zimmerman, B. A.: 1973, Astrophys. J. 184, 493.ADSCrossRefGoogle Scholar
  7. Cameron, A.G.W.: 1973, Space Sci. Rev. 15, 121.ADSCrossRefGoogle Scholar
  8. Caughlan, G. R.: 1965, Astrophys. J. 141, 688.ADSCrossRefGoogle Scholar
  9. Caughlan, G. R. and Fowler, W. A.: 1964, Astrophys. J. 139, 1180.ADSCrossRefGoogle Scholar
  10. Couch, R. G. and Arnett, W. D.: 1972, Astrophys. J. 178, 771.ADSCrossRefGoogle Scholar
  11. Dearborn, D.S.P., Eggleton, P. P., and Schramm, D. N.: 1976, Astrophys. J. 203, 455.ADSCrossRefGoogle Scholar
  12. Dearborn, D.S.P. and Schramm, D. D.: 1974, Astrophys. J. Letters 194, L67.ADSCrossRefGoogle Scholar
  13. Dyer, P.: 1973, in D. N. Schramm and W. D. Arnett (eds.), Explosive Nucleosynthesis, Univ. of Texas Press, Austin, p. 195.Google Scholar
  14. Dyer, P. and Barnes, C. A.: 1974, Nucl. Phys. A 233, 495.ADSCrossRefGoogle Scholar
  15. Edwards, A.: 1970, Monthly Notices Roy. Astron. Soc. 146, 445.ADSGoogle Scholar
  16. Fowler, W. A., Caughlan, G. R., and Zimmerman, B. A.: 1975, Ann. Rev. Astron. Astrophys. 13, 69.ADSCrossRefGoogle Scholar
  17. Fricke, K.: 1973, Astrophys. J. 183, 941.ADSCrossRefGoogle Scholar
  18. Howard, W. M., Arnett, W. D., and Clayton, D. D.: 1971, Astrophys. J. 165, 495.ADSCrossRefGoogle Scholar
  19. Hoyle, F. and Fowler, W. A.: 1960, Astrophys. J. 132, 565.ADSCrossRefGoogle Scholar
  20. Hoyle, F. and Fowler, W. A.: 1965, in I. Robinson, A. Schild, and E. L. Schucking (eds.), Quasi-Stellar Sources and Gravitational Collapse, Univ. of Chicago Press, Chicago, p. 17.Google Scholar
  21. Iben, I., Jr.: 1964, Astrophys. J. 140, 1631.ADSCrossRefGoogle Scholar
  22. Iben, I., Jr.: 1975a, Astrophys. J. 196, 525.ADSCrossRefGoogle Scholar
  23. Iben, I., Jr.: 1975b, Astrophys. J. 196, 549.ADSCrossRefGoogle Scholar
  24. Lazareff, B., Audouze, J., Starrfield, S., and Truran, J. W.: 1977, “Hot CNO-Ne Cycle Hydrogen Burning II. Explosive Hydrogen Burning” (in preparation).Google Scholar
  25. Rolfs, C. and Rodney, W. S.: 1974, Astrophys. J. Letters 194, L63.ADSCrossRefGoogle Scholar
  26. Scalo, J. M.: 1974, Astrophys. J. 194, 361.ADSCrossRefGoogle Scholar
  27. Schwarzschild, M. and Härm, R.: 1966, Astrophys. J. 145, 496.ADSCrossRefGoogle Scholar
  28. Schwarzschild, M. and Härm, R.: 1967, Astrophys. J. 150, 961.ADSCrossRefGoogle Scholar
  29. Shapiro, M. M. and Silberberg, R.: 1970, Ann. Rev. Nucl. Sci. 20, 323.ADSCrossRefGoogle Scholar
  30. Starrfield, S., Sparks, W. M., and Truran, J. W.: 1976, in P. P. Eggleton, S. Milton, and J. Whelan (eds.), “Evolution and Structure of Close Binaries”, IAU Symposium No. 73, D. Reidel Publishing Company, Dordrecht, Holland (in press).Google Scholar
  31. Starrfield, S., Truran, J. W., Sparks, W. M., and Kutter, G. S.: 1972, Astrophys. J. 176, 169.ADSCrossRefGoogle Scholar
  32. Sugimoto, D. and Nomoto, K.: 1975, Publ. Astron. Soc. Japan 27, 197.ADSGoogle Scholar
  33. Talbot, R. J. and Arnett, W. D.: 1973, Astrophys. J. 186, 69.ADSCrossRefGoogle Scholar
  34. Truran, J. W.: 1972, in H. R. Johnson, J. P. Mutschlecner, and B. F. Peery, Jr. (eds.), Red Giant Stars, Indiana Univ. Press, Bloomington, p. 394.Google Scholar
  35. Truran, J. W.: 1973, Comments Astrophys. Space Phys. 5, 117.ADSGoogle Scholar
  36. Truran, J. W. and Cameron, A.G.W.: 1971, Astrophys. Space Sci. 14, 179.ADSCrossRefGoogle Scholar
  37. Truran, J. W. and Iben, I., Jr.: 1977, “On s-Process Nucleosynthesis in Thermally Pulsing Stars” (in preparation).Google Scholar
  38. Ulrich, R. K.: 1973, in D. N. Schramm and W. D. Arnett (eds.), Explosive Nucleosynthesis, Univ. of Texas Press, Austin, p. 139.Google Scholar
  39. Wallerstein, G.: 1973, Ann. Rev. Astron. Astrophys. 11, 115.ADSCrossRefGoogle Scholar

Copyright information

© D. Reidel Publishing Company, Dordrecht-Holland 1977

Authors and Affiliations

  • James W. Truran
    • 1
  1. 1.Department of AstronomyUniversity of IllinoisUSA

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