Hostname: page-component-586b7cd67f-dsjbd Total loading time: 0 Render date: 2024-11-29T11:32:02.538Z Has data issue: false hasContentIssue false
  • English
  • Français

Planetary Nebulae and Chemical Evolution of the Galaxy

Published online by Cambridge University Press:  22 September 2016

Beatrice M. Tinsley
Beatrice M. Tinsley*
Affiliation:
Yale University Observatory

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The chemical evolution of galaxies is controlled by star formation, stellar mass loss, gas flows, and the compositions of matter involved in these processes. Planetary nebulae (PN) thus affect chemical evolution directly in representing mass ejection at the end of the nuclear burning lives of many stars, and in enriching the interstellar medium in elements that are overabundant in the nebulae. Supernovae often eclipse PN in discussions of these effects, so it is noteworthy that planetary precursor stars not only provide much of the present stellar mass loss in the solar neighborhood, but also show as clear evidence as supernova remnants for the ejection of elements newly synthesized in the stars themselves. Furthermore, PN are tracers of the past star formation history in a galaxy, since their rate of occurrence depends on the birthrate of progenitor stars during the whole lifetime of the system.

Type
Session VIII: Planetary Nebulae and Their Influence on the Galaxy
Information
Symposium - International Astronomical Union , Volume 76: Planetary Nebulae , 1978 , pp. 341 - 352
Copyright
Copyright © Reidel 1978 

References

Alloin, D., Cruz-Gonzalez, C., and Peimbert, M.: 1976, Astrophys. J. 205, 74.Google Scholar
Audouze, J. and Tinsley, B.M.: 1975, Ann. Rev. Astron. Astrophys. 14, 43.Google Scholar
Cahn, J.H. and Kaler, J.B.: 1971, Astrophys. J. Suppl. 22, 319.Google Scholar
Cahn, J.H. and Wyatt, S.P.: 1976, Astrophys. J. 210, 508.Google Scholar
Cox, D.P. and Smith, B.W.: 1976, Astrophys. J. 203, 361.Google Scholar
Cudworth, K.M.: 1974, Astron. J. 79, 1384.Google Scholar
Dearborn, D.S.: 1977, private communication.Google Scholar
Gordon, M.A. and Burton, W.B.: 1976, Astrophys. J. 208, 346.Google Scholar
Grieg, W.E.: 1971, Astron. Astrophys. 10, 161.Google Scholar
Larson, R.B.: 1972, Nature Phys. Sci. 236, 7.CrossRefGoogle Scholar
Mayor, M. and Martinet, L.: 1977, Astron. Astrophys. 55, 221.Google Scholar
Oort, J.H.: 1970, Astron. Astrophys. 7, 381.Google Scholar
Ostriker, J.P. and Peebles, P.J.E.: 1973, Astrophys. J. 186, 467.Google Scholar
Ostriker, J.P. and Thuan, T.X.: 1975, Astrophys. J. 202, 353.Google Scholar
Salpeter, E.E.: 1955, Astrophys. J. 121, 161.Google Scholar
Salpeter, E.E.: 1971, Ann. Rev. Astron. Astrophys. 9, 127.CrossRefGoogle Scholar
Schmidt, M.: 1959, Astrophys. J. 129, 243.Google Scholar
Schmidt, M.: 1975, Astrophys. J. 202, 22.Google Scholar
Tammann, G.A.: 1977, in Schramm, D.N. (ed.), Supernovae, D. Reidel Publ. Co., Dordrecht - Holland, p. 95.Google Scholar
Tinsley, B.M.: 1977a, in Schramm, D.N. (ed.), Supernovae, D. Reidel Publ. Co., Dordrecht - Holland, p. 117.Google Scholar
Tinsley, B.M.: 1977b, Astrophys. J. 215, in press.Google Scholar
Tinsley, B.M. and Ostriker, J.P.: 1976, in Contopoulos, G. (ed.), Reports on Astronomy, Vol. XVIA-Part 2, D. Reidel Publ. Co., Dordrecht - Holland, p. 161.Google Scholar
Torres-Peimbert, S. and Peimbert, M.: 1977, preprint.Google Scholar
Truran, J.W.: 1976, in Audouze, J. (ed.), CNO Isotopes in Astrophysics, D. Reidel Publ. Co., Dordrecht - Holland.Google Scholar