Figure 10. Luminosity of normal PWNe as a function of the rotational energy loss of their corresponding pulsars. Data presented as black dots are taken from Kargaltsev & Pavlov (2008), whereas the blue star represents the high-B source RRAT J1819−1458 (Rea et al. 2009b). The dashed line represents the ηX = 0.2 of RRAT J1819−1458, and the solid line represents the ηX = 0.7 of Swift J1834.9−0846. The three red dots represent the luminosity of the candidate MWN around Swift J1834.9−0846 at the detected epochs. (Figure adapted from Rea et al. 2009b.)
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