A lower limit for the birth rate of pulsars

Mathematics – Probability

Scientific paper

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Milky Way Galaxy, Probability Distribution Functions, Pulsars, Statistical Analysis, Stellar Evolution, Supernovae, Range (Extremes), Scale (Ratio)

Scientific paper

A lower limit for the birth rate of pulsars in the Galaxy is estimated, using experimental data on observed pulsars. Novel features of the approach employed are: (1) no pulsar model is assumed, and (2) selection effects are allowed for in a model-independent way. A mean birth rate of one pulsar per 18 years allows the projection with 95% confidence of a lower bound of 50 years. The calculation described reduces the discrepancy between pulsar and supernova birth rates.

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