Non-standard s -process in massive rotating stars Yields of 10-150 M ? models at Z = 10 -3 (2018)

First Author: Choplin A

Attributed to: Nuclear Physics Rolling Grant funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201833283

Publication URI: http://dx.doi.org/10.1051/0004-6361/201833283

Type: Journal Article/Review

Parent Publication: Astronomy & Astrophysics

ISSN: 1432-0746