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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Published in | Nature communications Vol. 12; no. 1; pp. 1025 - 11 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
London
Nature Publishing Group UK
15.02.2021
Nature Publishing Group Nature Portfolio |
Subjects | |
Online Access | Get full text |
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