Mass-loading of bow shock pulsar wind nebulae

We investigate the dynamics of bow shock nebulae created by pulsars moving supersonically through a partially ionized interstellar medium. A fraction of interstellar neutral hydrogen atoms penetrating into the tail region of a pulsar wind will undergo photo-ionization due to the UV light emitted by...

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Detalles Bibliográficos
Autores principales:	Morlino, Giovanni, Lyutikov, Maxim, Vorster, Michael
Formato:	Objeto de conferencia
Lenguaje:	Inglés
Publicado:	2015
Materias:	Ciencias Astronómicas bow shock nebulae pulsars ionized interstellar medium
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/167940
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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