Sarah Buchner (Hartebeesthoek Radio Astronomy Observatory)Vela Glitch Monitoring at HartRAO-- Sarah Buchner Colloquium |
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The Australia Telescope National Facility Colloquium | |||
15:00-16:00 Tue 24 Apr 2012 | |||
Marsfield Lecture Theatre |
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AbstractThe Vela pulsar, like many other young pulsars, undergoes occasional sudden ''spin-ups'' in rotational frequency known as glitches. These glitches are characterized by a sudden (less than 30s) rise in the rotation frequency accompanied by a jump in the spin-down of the pulsar. This is generally followed by rapidly decaying transients in the spin-down and a gradual linear recovery. This recovery provides insight into the internal structure of the neutron star.
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