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Ultra-heavy cosmic-ray science: Are r-process nuclei in the cosmic rays produced in supernovae or binary neutron star mergers?

Binns, Walter and Israel, M. ~H. and Rauch, B. ~F. and Cummings, A. ~C. and Davis, A. ~J. and Labrador, A. ~W. and Leske, R. ~A. and Mewaldt, R. ~A. and Stone, E. ~C. and Wiedenbeck, M. ~E. and Brandt, T. ~J. and Christian, E. ~R. and Link, J. ~T. and Mitchell, J. ~W. and de Nolfo, G. ~A. and von Rosenvinge, T. ~T. and Sakai, K. and Sasaki, M. and Waddington, C. ~J. and Janka, H. ~T. and Melott, A. ~L. and Mason, G. ~M. and Seo, E. -S. and Adams, J. ~H. and Thielemann, F. -K. and Heger, A. and Lugaro, M. and Westphal, A. ~J.. (2019) Ultra-heavy cosmic-ray science: Are r-process nuclei in the cosmic rays produced in supernovae or binary neutron star mergers? Bulletin of the American Astronomical Society, 51 (3). p. 313.

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Official URL: https://edoc.unibas.ch/75123/

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Faculties and Departments:05 Faculty of Science > Departement Physik > Former Organization Units Physics > Theoretische Physik Astrophysik (Thielemann)
UniBasel Contributors:Thielemann, Friedrich-Karl
Item Type:Article
Article Subtype:Research Article
Publisher:American Astronomical Society
ISSN:0002-7537
Note:Publication type according to Uni Basel Research Database: Journal article
Last Modified:01 Apr 2020 13:08
Deposited On:01 Apr 2020 13:08

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