Fast orbital shrinkage of black hole X-ray binaries driven by circumbinary disks
Recently, the black hole X-ray binary (BHXB) Nova Muscae 1991 has been reported to be experiencing an extremely rapid orbital decay. So far, three BHXBs have anomalously high orbital period derivatives, which can not be interpreted by the standard stellar evolution theory. In this work, we investiga...
| Príomhchruthaitheoirí: | , |
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| Formáid: | Journal article |
| Foilsithe / Cruthaithe: |
IOP Publishing
2019
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