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* Scientific Article * Impact Factor 6.630 |
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Ali Alazzawi, Sh.M., Abood, D.D., & Shneen, W.F.
Simulating the dynamic of supermassive black holes on the formation of dwarf galaxies. |
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Full Article: PDF
Scientific Object Identifier: http://s-o-i.org/1.1/TAS-09-161-1
DOI: https://dx.doi.org/10.15863/TAS.2026.09.161.1
Language: English
Citation: Ali Alazzawi, Sh.M., Abood, D.D., & Shneen, W.F. (2026). Simulating the dynamic of supermassive black holes on the formation of dwarf galaxies. ISJ Theoretical & Applied Science, 09 (161), 1-12. Soi: https://s-o-i.org/1.1/TAS-09-161-1 Doi: https://dx.doi.org/10.15863/TAS.2026.09.161.1 |
Pages: 1-12
Published: 30.09.2026
Abstract: This study explores the influence of supermassive black holes (SMBHs) on the formation and evolution of dwarf galaxies. It addresses the limited understanding of SMBH prevalence and their feedback effects in low-mass galactic environments. Using observational data from the Hubble Space Telescope (HST), Chandra X-ray Observatory, and the James Webb Space Telescope (JWST), along with spectroscopic analysis and computational simulations, the study examines SMBH signatures, star formation impacts, and structural effects. The methodology integrates multi-wavelength imaging and hydrodynamic modeling to assess how SMBHs regulate gas dynamics and star formation. Key findings suggest that SMBHs exist in many dwarf galaxies, influencing both galactic morphology and evolution through feedback processes. The results contribute to refining galaxy formation models by highlighting SMBH activity outside massive galaxies. Practical implications include improved SMBH detection in low-luminosity environments and enhanced simulation parameters for early-universe modeling. This research fills gaps in SMBH studies by aligning theoretical models with emerging observations, offering a new lens on galactic evolution and the role of black holes in the early cosmos.
Key words: Supermassive Black Holes, Dwarf Galaxies, Star Formation, Galaxy Evolution, Astrophysical Simulations.
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