A rapidly changing jet orientation in the stellar-mass black-hole system V404 Cygni
Powerful relativistic jets are one of the main ways in which accreting black holes provide kinetic feedback to their surroundings. Jets launched from or redirected by the accretion flow that powers them are expected to be affected by the dynamics of the flow, which for accreting stellar-mass black h...
| Κύριοι συγγραφείς: | , , , , , , , , , , , , , , , , , , , , |
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| Μορφή: | Journal article |
| Γλώσσα: | English |
| Έκδοση: |
Nature Research
2019
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| Θέματα: |