SILICON CARBIDE GRAINS OF TYPE C PROVIDE EVIDENCE FOR THE PRODUCTION OF THE UNSTABLE ISOTOPE 32 Si IN SUPERNOVAE (2013)

First Author: Pignatari M

Attributed to: Stellar Astrophysics at Keele funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1088/2041-8205/771/1/l7

Publication URI: http://dx.doi.org/10.1088/2041-8205/771/1/l7

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 1