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Modification Of the Sixth-Degree Polynomial of Rotational Angular Velocity and Mass of Some Spiral Barred Galaxies
Subject area: Physical Sciences and Environment · Area of research: Space Science
DOI: https://doi.org/10.64388/IREV9I9-1715202
Abstract
This work explores the intricate connection between the sixth polynomial of rotational velocity and the mass of particular spiral-barred galaxies. Using a comprehensive reworking of existing data and theoretical models, I aim to shed light on the dynamics behind these cosmic structures. Using complex MATLAB polynomial fitting techniques, the rotational curves of several galaxies were examined to assess the effect of their mass distributions on rotational angular velocity profiles. To better understand the spiral-barred galaxies under study, the data set was refined using Python to convert it to the appropriate units and then tabulated, which was utilized to construct MATLAB syntax. It was reviewed that there was a considerable correlation between the polynomial coefficients and the galaxies' morphological classifications, suggesting that the structural elements of spiral-barred galaxies have a significant impact on their rotational dynamics. The importance of polynomial representations in astrophysical modeling is highlighted in this work, which contributes to our understanding of galaxy formation and evolution. These spiral barred galaxies' mass and rotating angular velocity were analyzed, and it was shown that there are various interactions between the two variables at various polynomial degrees. Lastly, several spiral barred galaxies showed some link at degree one polynomial, but at another degree polynomial, there is no correlation between mass and rotating angular velocity at different reclassification groups.
Keywords
Barred Spiral Galaxies, Sixth-Degree Polynomial, Rotational Angular Velocity, Mass, And Data.
How to cite this paper
@article{1715202,
author = {Dr. Emmanuel Chiadi Ekwubiri},
title = {Modification Of the Sixth-Degree Polynomial of Rotational Angular Velocity and Mass of Some Spiral Barred Galaxies},
journal = {Iconic Research And Engineering Journals},
year = {2026},
volume = {9},
number = {9},
pages = {1860-1871},
issn = {2456-8880},
url = {https://www.irejournals.com/formatedpaper/1715202.pdf},
abstract = {This work explores the intricate connection between the sixth polynomial of rotational velocity and the mass of particular spiral-barred galaxies. Using a comprehensive reworking of existing data and theoretical models, I aim to shed light on the dynamics behind these cosmic structures. Using complex MATLAB polynomial fitting techniques, the rotational curves of several galaxies were examined to assess the effect of their mass distributions on rotational angular velocity profiles. To better understand the spiral-barred galaxies under study, the data set was refined using Python to convert it to the appropriate units and then tabulated, which was utilized to construct MATLAB syntax. It was reviewed that there was a considerable correlation between the polynomial coefficients and the galaxies' morphological classifications, suggesting that the structural elements of spiral-barred galaxies have a significant impact on their rotational dynamics. The importance of polynomial representations in astrophysical modeling is highlighted in this work, which contributes to our understanding of galaxy formation and evolution. These spiral barred galaxies' mass and rotating angular velocity were analyzed, and it was shown that there are various interactions between the two variables at various polynomial degrees. Lastly, several spiral barred galaxies showed some link at degree one polynomial, but at another degree polynomial, there is no correlation between mass and rotating angular velocity at different reclassification groups.},
keywords = {Barred Spiral Galaxies, Sixth-Degree Polynomial, Rotational Angular Velocity, Mass, And Data.},
month = {March},
doi = {https://doi.org/10.64388/IREV9I9-1715202}
}