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129I and 247Cm in meteorites constrain the last astrophysical source of solar r-process elements. (2021)

First Author: Côté B

Attributed to: Astrophysics at The University of Hull funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1126/science.aba1111

PubMed Identifier: 33632846

Publication URI: http://europepmc.org/abstract/MED/33632846

Type: Journal Article/Review

Volume: 371

Parent Publication: Science (New York, N.Y.)

Issue: 6532

ISSN: 0036-8075