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Scintillation measurements of the millisecond pulsar PSR J0030+0451\n and pulsar space velocities

L. NicastroIstituto di Fisica Cosmica con Applicazioni all'Informatica , CNR , Via U. La Malfa 153 , 90146 Palermo , ItalyF. NigroOsservatorio Astronomico di Bologna , Via Ranzani 1 , 40127 Bologna , ItalyN. D’AmicoOsservatorio Astronomico di Bologna , Via Ranzani 1 , 40127 Bologna , ItalyV. LumiellaDipartimento di Astronomia, Università degli Studi di Bologna, Via Ranzani 1, 40127 Bologna, ItalyS. JohnstonResearch Centre for Theoretical Astrophysics, University of Sydney, NSW 2006, Australia
2001en
ABI

Annotatsiya

\n \nScintillation observations of the nearby single millisecond pulsar (MSP) PSR J0030+0451 \nwere carried out with the Parkes 64 m radiotelescope at three different \nepochs in 1999.\nFrom analysis of the dynamic spectrum we obtained the amplitude of the\nelectron density power \nspectrum $\\log \\overline{C_{\\rm N}^2} \\simeq -3.33$ and a scintillation velocity \n$V_{\\rm iss} \\la 15$ km s-1. \nThis result shows that the Shklovskii effect on the spin-down \nrate $\\dot P$ is negligible. We also performed a correlation analysis\nbetween pulsar proper motions (Vpm) and scintillation velocities\n(Viss) using updated measurements for a sample of 77 objects,\n17 of which are MSPs.\nThe full sample shows a correlation coefficient $r_{\\rm s} \\simeq 80\\%$ at an\nextremely high significance level, while for the\nMSP sub-sample (excluding 2 outliers) we obtain $r_{\\rm s} \\simeq 90\\%$.\n\n \n

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