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

Author: Hirschi R.   Maeder A.  

Publisher: Edp Sciences

E-ISSN: 1432-0746|519|issue|A16-A16

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.519, Iss.issue, 2010-09, pp. : A16-A16

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract