Assertion: pulsar's field | /r/CapableOf | keep the gas
Facets:
value: before the burst
type: TEMPORAL
Source sentences:
text: Before the burst, the fast spinning magnetic field of the neutron star (blue arrow) keeps the gas (white arrows) flowing from the companion star at bay, preventing it from reaching closer to the neutron star and effectively creating an inner edge at the center of the disc.
text: According to one model, type-II bursts occur because the fast spinning magnetic field of the neutron star keeps the gas flowing from the companion star at bay, preventing it from reaching closer to the neutron star and effectively creating an inner edge at the center of the disc.