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• W3103608919 abstract "We take a fresh look at the determination of distances and velocities of neutron stars. The conversion of a parallax measurement into a distance, or distance probability distribution, has led to a debate quite similar to the one involving Cepheids, centering on the question whether priors can be used when discussing a single system. With the example of PSRJ0218+4232 we show that a prior is necessary to determine the probability distribution for the distance. The distance of this pulsar implies a gamma-ray luminosity larger than 10% of its spindown luminosity. For velocities the debate is whether a single Maxwellian describes the distribution for young pulsars. By limiting our discussion to accurate (VLBI) measurements we argue that a description with two Maxwellians, with distribution parameters sigma1=77 and sigma2=320 km/s, is significantly better. Corrections for galactic rotation, to derive velocities with respect to the local standards of rest, are insignificant." @default.
• W3103608919 created "2020-11-23" @default.
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• W3103608919 date "2017-09-01" @default.
• W3103608919 modified "2023-10-16" @default.
• W3103608919 title "A New Look at Distances and Velocities of Neutron Stars" @default.
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• W3103608919 doi "https://doi.org/10.1007/s12036-017-9474-5" @default.
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