Numerical simulations of mass loading in the tails of bow-shock pulsar-wind nebulae
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DOI: 10.1093/mnras/sty2525
Abstract: When a pulsar is moving through a partially ionized medium, a fraction of neutral Hydrogen atoms penetrate inside the pulsar wind and can be photo-ionized by the nebula UV radiation. The resulting protons remains attached… read more here.
Keywords: pulsar; numerical simulations; tails bow; pulsar wind ... See more keywords