Observations of binary stars containing an accreting black hole or neutron star often show x-ray emission extending to high energies (>10 kilo–electron volts), which is ascribed to an accretion disk corona of energetic particles akin to those seen in the solar corona. Despite their ubiquity, the physical conditions in accretion disk coronae remain poorly constrained.
[2]
Original Source [3]
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Links:
[1] http://admin.indiaenvironmentportal.org.in/feature-article/precise-measurement-magnetic-field-corona-black-hole-binary-v404-cygni
[2] http://www.indiaenvironmentportal.org.in/files/file/black_hole.pdf
[3] http://science.sciencemag.org/content/358/6368/1299/tab-pdf
[4] http://admin.indiaenvironmentportal.org.in/category/author/yigit-dallilar
[5] http://admin.indiaenvironmentportal.org.in/category/author/stephen-s-eikenberry
[6] http://admin.indiaenvironmentportal.org.in/category/author/alan-garner
[7] http://admin.indiaenvironmentportal.org.in/category/journal/science
[8] http://admin.indiaenvironmentportal.org.in/category/thesaurus/physical-science
[9] http://admin.indiaenvironmentportal.org.in/category/thesaurus/astronomy
