From Be X-Ray Binaries to Double Neutron Stars: Exploring the Spin and Orbital Evolution

We explore the evolutionary link between Galactic Be X-ray binaries (BeXBs) and Galactic field double neutron stars (DNSs) based on the properties of the NS spin period—<i>P</i> and binary orbital period—<inline-formula><math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><semantics><ms...

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Detalles Bibliográficos

Principais autores:	Yungang Zhou, Dehua Wang, Chengmin Zhang
Formato:	Artigo
Idioma:	Inglês
Publicado:	MDPI AG 2025-02-01
Series:	Universe
Assuntos:	pulsar binary pulsar Be X-ray binary double neutron star
Acceso en liña:	https://www.mdpi.com/2218-1997/11/2/51
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