Accretion Spin-up and a Strong Magnetic Field in the Slow-spinning Be X-Ray Binary MAXI J0655-013

Accretion Spin-up and a Strong Magnetic Field in the Slow-spinning Be X-Ray Binary MAXI J0655-013

We present Monitor of All-sky X-ray Image (MAXI) and Nuclear Spectroscopic Telescope Array (NuSTAR) observations of the Be X-ray binary, MAXI J0655−013, in outburst. NuSTAR observed the source once early in the outburst, when spectral analysis yields a bolometric (0.1–100 keV), unabsorbed source lum...

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Detalhes bibliográficos
Principais autores: Sean N. Pike, Mutsumi Sugizaki, Jakob van den Eijnden, Benjamin Coughenour, Amruta D. Jaodand, Tatehiro Mihara, Sara E. Motta, Hitoshi Negoro, Aarran W. Shaw, Megumi Shidatsu, John A. Tomsick
Formato: Artigo
Idioma:English
Publicado em: IOP Publishing 2023-01-01
coleção:The Astrophysical Journal
Assuntos:
High-mass x-ray binary stars
Neutron stars
Accretion
Pulsars
Acesso em linha:https://doi.org/10.3847/1538-4357/ace696

Internet

https://doi.org/10.3847/1538-4357/ace696

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