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

First Author: Hirschi R

Attributed to: Stellar Astrophysics at Keele funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/201014222

Publication URI: http://dx.doi.org/10.1051/0004-6361/201014222

Type: Journal Article/Review

Parent Publication: Astronomy and Astrophysics