Hostname: page-component-7857688df4-8d8b9 Total loading time: 0 Render date: 2025-11-17T20:39:54.378Z Has data issue: false hasContentIssue false
  • English
  • Français

Heavy Element Abundances in the Magellanic Clouds

Published online by Cambridge University Press:  25 April 2016

Stephen C. Russell
Stephen C. Russell*
Affiliation:
School of Cosmic Physics, Dublin Institute for Advanced Studies, 5 Merrion Square, Dublin 2, Ireland
Get access Rights & Permissions [Opens in a new window]

Abstract

This paper presents a brief discussion of the apparent underdepletion of the heavy neutron-capture elements (elements heavier than Ba), compared with Fe in the Magellanic Clouds. The s-process appears to have been only effective in forming elements in the light neutron-capture group (Sr, Y, Zr) in the Magellanic Clouds, but to have much reduced effectiveness in forming the heavy neutron-capture group. The abundances of the elements heavier than Ba have a distribution that indicates that they were produced by the r-process alone.

Information

Type
Extragalactic
Information
Publications of the Astronomical Society of Australia , Volume 9 , Issue 1 , 1991 , pp. 82 - 83
Copyright
Copyright © Astronomical Society of Australia 1991

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

Article purchase

Temporarily unavailable

References

Cameron, A. G. W., 1982a, Astrophys. Space Sci., 82, 123.CrossRefGoogle Scholar
Gilroy, K. K., Sneden, C., Pilachowski, C. A. and Cowan, J. J., 1988, Astrophys. J., 327, 298.Google Scholar
Malaney, R. A., 1987a, Astrophys. J., 321, 832.Google Scholar
Malaney, R. A., 1987b, Astrophys. Space Sci., 137, 251.Google Scholar
Russell, S.C. and Bessell, M. S., 1989, Astrophys. J. Suppl. Ser., 70, 865.Google Scholar
Russell, S.C. and Dopita, M. A., 1990a, Astrophys. J. Suppl. Ser., in press.Google Scholar
Russell, S.C. and Dopita, M. A., 1990b, Astrophys. J., submitted.Google Scholar
Spite, F., Spite, M. and Francois, P., 1989, Astron. Astrophys., 210, 25.Google Scholar
Truran, J. W., 1981, Astron. Astrophys., 97, 391.Google Scholar
Wheeler, J. C., Sneden, C. and Truran, J. W., 1989, Annu. Rev. Astron. Astrophys., 27, 279.Google Scholar