Discover
/
Article

Evolution of red‐giant stars

JAN 01, 1976
Thermal instabilities in helium‐burning shells are linked to the origin of certain elements heavier than iron—in one star the surface abundances of these elements increased by 25 times in the last ten years.

DOI: 10.1063/1.3023252

Allen V. Sweigart

Theorists are paying a lot of attention nowadays to the structure and evolution of highly luminous stars with low surface temperatures. These stars, referred to as “red giants” because of their color and large radii, are believed to be in an advanced phase of their evolution. Most stars pass through at least one such phase, late in their lifetimes—as will our Sun.

References

  1. 1. E. M. Burbidge, G. R. Burbidge, W. A. Fowler, F. Hoyle, Rev. Mod. Phys. 29, 547 (1957).https://doi.org/RMPHAT

  2. 2. G. Wallerstein, Ann. Rev. Astron. and Astrophys. 11, 115 (1973).https://doi.org/ARAAAJ

  3. 3. J. W. Truran, in Proceedings of the Conference on Red Giant Stars (H. R. Johnson, J. P. Mutschlecner, B. F. Peery, eds.), Bloomington, Indiana, page 394 (1973).

  4. 4. G. E. Langer, R. P. Kraft, K. S. Anderson, Astrophys. J. 189, 509 (1974).https://doi.org/ASJOAB

  5. 5. M. Schwarzschild, R. Härm, Astrophys. J. 142, 855 (1965).https://doi.org/ASJOAB

  6. 6. A. Weigert, Z. Astrophys. 64, 395 (1966).https://doi.org/ZEASAJ

  7. 7. M. Schwarzschild, R. Härm, Astrophys. J. 150, 961 (1967).https://doi.org/ASJOAB

  8. 8. B. Paczyński, Acta Astron. 21, 417 (1971).https://doi.org/AASWAM

  9. 9. I.‐J. Sackmann, K. H. Despain, Astrophys. J. 189, 523 (1974).https://doi.org/ASJOAB

  10. 10. I. IbenJr, Astrophys. J. 196, 525 (1975).https://doi.org/ASJOAB

  11. 11. R. A. Gingold, Astrophys. J. 193, 177 (1974).https://doi.org/ASJOAB

  12. 12. R. H. Sanders, Astrophys. J. 150, 971 (1967).https://doi.org/ASJOAB

  13. 13. A. G. W. Cameron, W. A. Fowler, Astrophys. J. 164, 111 (1971).https://doi.org/ASJOAB

  14. 14. J. M. Scalo, R. K. Ulrich, Astrophys. J. 183, 151 (1973).https://doi.org/ASJOAB

  15. 15. E. H. Levy, W. K. Rose, Astrophys. J. 193, 419 (1974).https://doi.org/ASJOAB

  16. 16. O. J. Eggen, Astrophys. J. 177, 489 (1972).https://doi.org/ASJOAB

  17. 17. A. V. Sweigart, Astrophys. J. 189, 289 (1974).https://doi.org/ASJOAB

  18. 18. A. V. Sweigart, Astrophys. J. 168, 79 (1971).https://doi.org/ASJOAB

More about the Authors

Allen V. Sweigart. Yale University Observatory, New Haven, Connecticut.

This Content Appeared In
pt-cover_1976_01.jpeg

Volume 29, Number 1

Related content
/
Article
Technical knowledge and skills are only some of the considerations that managers have when hiring physical scientists. Soft skills, in particular communication, are also high on the list.
/
Article
Professional societies can foster a sense of belonging and offer early-career scientists opportunities to give back to their community.
/
Article
Interviews offer a glimpse of how physicists get into—and thrive in—myriad nonacademic careers.
/
Article
Research exchanges between US and Soviet scientists during the second half of the 20th century may be instructive for navigating today’s debates on scientific collaboration.

Get PT in your inbox

Physics Today - The Week in Physics

The Week in Physics" is likely a reference to the regular updates or summaries of new physics research, such as those found in publications like Physics Today from AIP Publishing or on news aggregators like Phys.org.

Physics Today - Table of Contents
Physics Today - Whitepapers & Webinars
By signing up you agree to allow AIP to send you email newsletters. You further agree to our privacy policy and terms of service.