Optical Characteristics of Electromagnetic Radiation, Emitted by Particles or Stars Moving near Supermassive Black Hole
The general problem of calculating of the propagation of electromagnetic radiation from particles or stars moving in the vicinity of a supermassive black hole is considered in geometrical optics approximation within the framework of the general theory of relativity. Different approaches that can be...
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| Format: | Article |
| Language: | English |
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MDPI AG
2021-08-01
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| Series: | Galaxies |
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| Online Access: | https://www.mdpi.com/2075-4434/9/3/57 |