Published 1990
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Cosmic Ray Elemental Abundances for 26<Z<40 Measured on HEAO-3
Abstract
Abundances relative to _(96)Fe have been derived for elements with charge, 2, in the range 32≤z≤40. With a resolution better than 0.5 charge unit at Z=38, we resolve _(37)Rb from _(38)Sr and use the Rb/Sr ratio to place a limit on the r-proccss enhancement of the cosmic ray source material in this charge range.
Additional Information
© Organizing Committee of the 21st Int. Cosmic Ray Conf. Provided by the NASA Astrophysics Data System. This work was supported in part by NASA grants NAG 8- 498, 500, and 502; and NGR 05-002-160, 24-005-050, and 26-008-001.Attached Files
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Additional details
- Eprint ID
- 45581
- Resolver ID
- CaltechAUTHORS:20140507-141130693
- NASA
- NAG8-498
- NASA
- NAG8-500
- NASA
- NAG8-502
- NASA
- NGR 05-002-160
- NASA
- NGR 24-005-050
- NASA
- NGR 26-008-001
- Created
-
2014-05-07Created from EPrint's datestamp field
- Updated
-
2020-03-09Created from EPrint's last_modified field
- Caltech groups
- Space Radiation Laboratory
- Other Numbering System Name
- Space Radiation Lab
- Other Numbering System Identifier
- 1989-07