On the angular momentum of the neutron star

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dc.creatorSeidov, Zakir F.
dc.date2003-10-20
dc.date.accessioned2026-07-07T02:10:41Z
dc.date.available2026-07-07T02:10:41Z
dc.descriptionIt is shown that the mass loss due to rotation-driven hydrodynamical instability during the catastrophic collapse of the star is small. Neutron star is formed with a large rotational kinetic energy and the spin-down takes place in the following life of neutron star as a pulsar.
dc.description3 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0310573
dc.identifierhttp://arxiv.org/abs/astro-ph/0310573
dc.identifier1970ATsir..567...3S
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6816
dc.subjectAstrophysics
dc.titleOn the angular momentum of the neutron star
dc.typetext

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