"Comptonizations" Example Sentences
1. The observed spectra of distant galaxies show evidence of comptonizations.
2. The study of comptonizations is important for understanding the behavior of photons in extreme environments.
3. The temperature profiles of corona can be determined by analyzing comptonizations.
4. Comptonizations in accretion disks of black holes can produce high-energy X-rays.
5. Theoretical models predict that comptonizations could affect the chemical composition of stellar atmospheres.
6. The presence of comptonizations can cause significant distortions in the observed spectra of supernovae.
7. The effects of comptonizations on cosmic microwave background radiation can provide valuable insights into the early universe.
8. Detailed analysis of comptonizations can help constrain the properties of dark matter particles.
9. Comptonizations in the atmospheres of neutron stars can lead to the formation of unexpected chemical compounds.
10. The phenomenon of comptonizations is a key tool for studying the properties of strong gravitational fields in the vicinity of black holes.
11. Observations of comptonizations in star-forming regions can provide clues about the origins of complex organic molecules.
12. The nature of comptonizations in the interstellar medium remains one of the most challenging questions in astrophysics.
13. The presence of comptonizations can cause significant uncertainties in the measurements of the cosmic microwave background radiation.
14. Comptonizations in the surroundings of pulsars can produce detectable gamma-ray emissions.
15. The study of comptonizations can help reveal the structure and dynamics of plasma flows in astrophysical systems.
16. Understanding the mechanisms of comptonizations is crucial for interpreting the observed properties of gamma-ray bursts.
17. Theoretical calculations of comptonizations in the atmospheres of brown dwarfs can explain the observed spectra of these objects.
18. Observations of comptonizations in active galactic nuclei can provide insights into the physical processes governing their emission.
19. The presence of comptonizations can affect the propagation of cosmic rays through the intergalactic medium.
20. The effects of comptonizations on the properties of the interstellar medium can have important implications for the formation and evolution of galaxies.
21. Comptonizations in the atmosphere of the Sun can cause significant disturbances in radio communications on Earth.
22. Theoretical models of comptonizations can explain the observed properties of gamma-ray bursts associated with supernovae.
23. The presence of comptonizatons in massive stars can significantly impact their evolutionary paths.
24. Observations of comptonizations in the vicinity of supermassive black holes can provide clues about their growth and evolution.
25. The study of comptonizations in active galactic nuclei is one of the most active areas of research in modern astrophysics.
26. Theoretical calculations of comptonizations in the magnetospheres of neutron stars can explain their observed X-ray emissions.
27. Comptonizations in the atmospheres of white dwarfs can produce unexpected spectral features that challenge current models.
28. The effects of comptonizations on the properties of cosmic rays can have important implications for their contribution to the energy density of the universe.
29. Observations of comptonizations in the vicinity of neutron stars can reveal the presence of strong magnetic fields.
30. The nature of comptonizations in black hole accretion disks is a major topic of research in theoretical astrophysics.
Common Phases
1. The comptonization process involves the scattering of photons by electrons;
2.
Comptonizations are often observed in astrophysics as a way to study the properties of hot plasmas;
3. The spectral features of comptonized radiation depend on the temperature and density of the plasma;
4. One of the most important applications of comptonization is in the study of black holes;
5. The comptonization of radiation is an important process in the formation of cosmic microwave background radiation.