Pulsar-Driven Jets in Supernovae, Gamma-Ray Bursts, and the Universe

Figure 10

Left, lower horizontal axis: the population of 497 pulsars from the Parkes Multibeam Survey which fall into binned distances, with centers between ~2.5 and ~10.75 kpc, plotted against the log of the product of their 1400 MHz fluxes and their NE2001 distances from [69, 70]. Right, upper horizontal axis: the same for a synthetic distribution of pulsars which obey the inverse square law. The two families of curves are both in order of increasing distance from left to right at a population fraction of 0.2.