The GSF instability and turbulence do not account for the relatively low rotation rate of pulsars (2010)

First Author: {Hirschi}, R. And {Maeder}, A.

Attributed to: Stellar Astrophysics at Keele funded by STFC

Abstract

No abstract provided

Bibliographic Information

Volume: 519

Parent Publication: \aap

Issue: 1004.5470