Measuring the Size of the Vela Pulsar’s Radio Emission Region

We describe the expected distribution of intensity for a scintillating source of finite size observed through a scattering medium, including systematic and instrumental effects. We describe measurements of the size of the Vela pulsar, using this technique.

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Published in:International Astronomical Union Colloquium 2000, Vol.177, p.211-214
Main Authors: Gwinn, C.R., Reynolds, J.E., Jauncey, D.L., Hirabayashi, H., Kobayashi, H., Murata, Y., Edwards, P.G., Carlson, B., Dougherty, S., Rizzo, D. Del, Britton, M.C., McCulloch, RM, Lovell, J.E.J.
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container_title International Astronomical Union Colloquium
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creator Gwinn, C.R.
Reynolds, J.E.
Jauncey, D.L.
Hirabayashi, H.
Kobayashi, H.
Murata, Y.
Edwards, P.G.
Carlson, B.
Dougherty, S.
Rizzo, D. Del
Britton, M.C.
McCulloch, RM
Lovell, J.E.J.
description We describe the expected distribution of intensity for a scintillating source of finite size observed through a scattering medium, including systematic and instrumental effects. We describe measurements of the size of the Vela pulsar, using this technique.
doi_str_mv 10.1017/S0252921100059492
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title Measuring the Size of the Vela Pulsar’s Radio Emission Region
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