Abstract
THE problem of the surprisingly high abundance of galactic helium which has been observed1,2 was the stimulus for this work. This communication proposes a new mechanism for rapid mass ejection from highly evolved stars. The mechanism is effective only over a specific, relatively short period of time in the life of the star. The general problem of mass loss from stars is the subject of an excellent review by Weymann3.
This is a preview of subscription content, access via your institution
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Buy this article
- Purchase on Springer Link
- Instant access to full article PDF
Prices may be subject to local taxes which are calculated during checkout
Similar content being viewed by others
References
Hoyle, F., and Tayler, R. G., Nature, 203, 1108 (1964).
Truran, J., Hansen, C. F., and Cameron, A. G. W., Astro. J., 70, 149 (1965).
Weymann, R., Ann. Rev. Astro. and Astrophys., 1, 97 (1963).
Schwarzschild, M., Structure and Evolution of the Stars (Princeton University Press, 1958).
Iben, I., Astrophys. J., 142, 1447 (1965).
Kippenhahn, R., et al., Zeit. f. Astrophysik, 61, 241 (1965).
Hayashi, C., Hoshi, R., and Sugimoto, D., Prog. Theor. Phys., 34, 885 (1965).
Greyber, H. D., Pennington, R., Wheeler, J. A., et al., Princeton University Report PM(B)-38 (Princeton, N.J., 1953).
Greyber, H. D., Rev. Mod. Phys., 30, 1068 (1958).
Fermi, E., and von Neumann, J., John von Neumann—Collected Works, 6, 431 (Pergamon Press, Oxford, 1963).
Fowler, W. A., Burbidge, E. M., Burbidge, G. R., and Hoyle, F., Astrophys. J., 142, 423 (1965).
Wallerstein, G., Astrophys. J., 142, 1260 (1965).
Deeming, T. J., Publ. Astro. Soc. Pacific, 77, 443 (1965).
Kopal, Z., Astrophys. Norvegica, 9, 239 (1964).
Hoffleit, D., and Smith, H. J., Nature, 198, 650 (1963).
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
GREYBER, H. Mass Ejection by Highly Evolved Stars. Nature 210, 510–511 (1966). https://doi.org/10.1038/210510a0
Issue Date:
DOI: https://doi.org/10.1038/210510a0
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.
