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Retrograde Accretion Disks in High-Mass Be/X-ray Binaries
We have compiled a comprehensive library of all X-ray observations of Magellanic pulsars carried out by XMM-Newton, Chandra, and RXTE in the period 1997–2014. In this work, we use the data from 53 high-mass Be/X-ray binaries in the Small Magellanic Cloud to demonstrate that the distribution of spin-...
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| Publicado no: | Mon Not R Astron Soc Lett |
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| Main Authors: | , , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
2017
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| Assuntos: | |
| Acesso em linha: | https://ncbi.nlm.nih.gov/pmc/articles/PMC7398147/ https://ncbi.nlm.nih.gov/pubmed/32747860 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1093/mnrasl/slx058 |
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