Insight-HXMT observations of jet-like corona in a black hole X-ray binary MAXI J1820+070
A black hole X-ray binary produces hard X-ray radiation from its corona and disk when the accreting matter heats up. During an outburst, the disk and corona co-evolves with each other. However, such an evolution is still unclear in both its geometry and dynamics. Here we report the unusual decrease...
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Veröffentlicht in: | arXiv.org 2021-03 |
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Format: | Artikel |
Sprache: | eng |
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