A model of two-stream non-radial accretion for binary X-ray pulsars

DOI10.1007/BF00651444zbMath0533.76043MaRDI QIDQ789951

V. M. Lipunov

Publication date: 1982

Published in: Astrophysics and Space Science (Search for Journal in Brave)

zbMATH Keywords

pulsarsneutron star evolutionnon-radial accretionspin time variationtwo-stream modelX-ray binary systems

Mathematics Subject Classification ID

Hydrodynamic and hydromagnetic problems in astronomy and astrophysics (85A30) Stability and instability of geophysical and astrophysical flows (76E20)

Related Items (1)

The ecology of rotators

This page was built for publication: A model of two-stream non-radial accretion for binary X-ray pulsars