The Origin of Radio Emission in Black Hole X-ray Binaries
We studied the relation of accretion-jet power and disk luminosity, especially the jet efficiencies and disk radiative efficiencies for different accretion disks as well as black hole (BH) spin, in order to explore the origin of radio emission in black hole X-ray binaries (BHXBs). We found that jet...
| Hoofdauteurs: | , , , |
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| Formaat: | Artikel |
| Taal: | English |
| Gepubliceerd in: |
MDPI AG
2021-10-01
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| Reeks: | Galaxies |
| Onderwerpen: | |
| Online toegang: | https://www.mdpi.com/2075-4434/9/4/78 |