Magnetic field decay in black widow pulsars

We study in this work the evolution of the magnetic field in 'redback-black widow' pulsars. Evolutionary calculations of these 'spider' systems suggest that first the accretion operates in the redback stage, and later the companion star ablates matter due to winds from the recycl...

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Detalles Bibliográficos
Autores principales:	Mendes, Camile, de Avellar, Marcio G. B., Horvath, J. E., Souza, Rodrigo A. de, Benvenuto, Omar Gustavo, De Vito, María Alejandra
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2018
Materias:	Ciencias Astronómicas Accretion discs Magnetic field Stars: neutron
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/93685 https://academic.oup.com/mnras/article/475/2/2178/4817548
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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