New model of relativistic slowly rotating neutron stars with surface layer crust: Application to giant glitches of Vela Pulsar

  1. González-Romero, L.M.
  2. Blázquez-Salcedo, J.L.
Konferenzberichte:
Journal of Physics: Conference Series

ISSN: 1742-6596,  1742-6588

Datum der Publikation: 2011

Ausgabe: 314

Nummer: 1

Art: Konferenz-Beitrag

DOI: 10.1088/1742-6596/314/1/012088 GOOGLE SCHOLAR
Datenquelle: Scopus