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Fig. 5.

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Probability for a selection of 30 known pulsars within 2 kpc to be found inside their parent environments, as a function of their characteristic ages. This is based on a Galactic population model made of a proper mix of isolated and cluster massive-star progenitors (see text), and a kick velocity distribution from Igoshev (2020). Dashed and dotted lines mark the 80% and 20% probabilities, respectively.

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