TESTING THE FALL-BACK DISK MODEL FOR RADIO PULSARS USING NEW DATA

DOI10.1142/S0218271804005110zbMath1057.85506MaRDI QIDQ4832429

Sevinç O. Tagieva

Publication date: 4 January 2005

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

zbMATH Keywords

neutron star

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15)

Related Items (1)

Temporal evolution of isolated pulsars; Age-Tau problem

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