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