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A Striking Confluence Between Theory and Observations of High-Mass X-ray Binary Pulsars
We analyse the most powerful X-ray outbursts from neutron stars in ten Magellanic high-mass X-ray binaries and three pulsating ultraluminous X-ray sources. Most of the outbursts rise to L(max) which is about the level of the Eddington luminosity, while the rest and more powerful outbursts also appea...
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| Pubblicato in: | Res Astron Astrophys |
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| Autori principali: | , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
2018
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| Soggetti: | |
| Accesso online: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6999737/ https://ncbi.nlm.nih.gov/pubmed/32021612 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1088/1674-4527/18/10/128 |
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