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...
Main Author: | Stanislav Komarov |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2021-08-01
|
Series: | Galaxies |
Subjects: | |
Online Access: | https://www.mdpi.com/2075-4434/9/3/57 |
Similar Items
-
A Candidate Runaway Supermassive Black Hole Identified by Shocks and Star Formation in its Wake
by: Pieter van Dokkum, et al.
Published: (2023-01-01) -
Probing the Mass Relation between Supermassive Black Holes and Dark Matter Halos at High Redshifts by Gravitational Wave Experiments
by: Kazuya Furusawa, et al.
Published: (2023-01-01) -
Meet the Parents: The Progenitor Binary for the Supermassive Black Hole Candidate in E1821+643
by: James Paynter, et al.
Published: (2023-01-01) -
Probing Supermassive Black Hole Seed Scenarios with Gravitational-wave Measurements
by: John Ellis, et al.
Published: (2024-01-01) -
A Candidate Supermassive Black Hole in a Gravitationally Lensed Galaxy at Z ≈ 10
by: Orsolya E. Kovács, et al.
Published: (2024-01-01)