A highly resistive layer withi. The crust of X-ray pulsars limits their spin periods

  1. Pons, J.A.
  2. Viganò, D.
  3. Rea, N.
Revue:
Nature Physics

ISSN: 1745-2481 1745-2473

Année de publication: 2013

Volumen: 9

Número: 7

Pages: 431-434

Type: Article

DOI: 10.1038/NPHYS2640 GOOGLE SCHOLAR