Comparative Study Between Rotational Angular Velocity of Some Spiral Barred Galaxies with Mass

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@article{1715556,
      author = {Ekwubiri, E. C.},
      title = {Comparative Study Between Rotational Angular Velocity of Some Spiral Barred Galaxies with Mass},
      journal = {Iconic Research And Engineering Journals},
      year = {2026},
      volume = {9},
      number = {9},
      pages = {2659-2669},
      issn = {2456-8880},
      url = {https://www.irejournals.com/formatedpaper/1715556.pdf},
      abstract = {A lot of emphasis has been paid to the disparity in galaxy rotation, which has led to research on the relationship between mass and radius and the rotating angular velocity of some spiral-barred galaxies. An alternate approach is required because of the morphologies of galaxies. The rotating angular velocities of these spiral-barred galaxies are not currently matched by classifications. The purpose of this study was to reclassify spiral-barred galaxies and establish the correlation between the mass and radius of eighty-four spiral-barred galaxies and their rotating angular velocities. The software used to examine 84 spiral-barred galaxies is Math Lab, Visual Studio, and Python. Information from the National Aeronautics and Space Administration (NASA) and the Internet was utilized to calculate the rotating angular velocity, specific angular momentum, and angular momentum. A Python calculation tool was written using these parameter values and the rotating angular velocity formulae. The results were presented alongside data from the internet along with their units. Among the findings for rotational angular velocity produced for eighty-four spiral barred galaxies are Butterfly Nebula = 2 km/s and Black Eye = 1.17E+03 km/s. The polynomials of spiral-barred galaxies were shown to behave more abnormally in comparison to their groups at higher degrees. It was discovered that at degree one, polynomial groups A and C showed an increasing correlation with rotational angular velocity and mass based on grouped classifications of spiral barred galaxies. Groups B and D, on the other hand, showed a partial retrogressive correlation with mass and rotating angular velocity. In conclusion, the relationship between mass and rotating angular velocity is either nonexistent or very weak.},
      keywords = {Spiral Barred Galaxies, Butterfly Nebula, Black eye, Galaxies, Spiral Galaxies},
      month = {March},
  }