Swift observations of V404 Cyg during the 2015 outburst: X-ray outflows from super-Eddington accretion
The black hole (BH) binary V404 Cyg entered the outburst phase in 2015 June after 26 yr of X-ray quiescence, and with its behaviour broke the outburst evolution pattern typical of most BH binaries. We observed the entire outburst with the Swift satellite and performed timeresolved spectroscopy of it...
| Main Authors: | , , , , , , , , , , , , , |
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| Format: | Journal article |
| Published: |
Oxford University Press
2017
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