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Font, J., Beckman, J.E., Martínez-Valpuesta, I., Borlaff, A.S., James, P.A., Díaz-García, S., et al. (2017) Kinematic Clues to Bar Evolution for Galaxies in the Local Universe: Why the Fastest Rotating Bars Are Rotating Most Slowly. The Astrophysical Journal, 835, Article No. 279.
https://doi.org/10.3847/1538-4357/835/2/279

has been cited by the following article:

• TITLE: Formation and Evolution of Galaxies: Starlight Synthesis Algorithm

  AUTHORS: Nick Barua

  KEYWORDS: Galaxies, Physics, Nuclei Kinematics, Galactic Nuclei, Active Nuclei, Velocity Dispersion

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.12 No.1, March 3, 2022

  ABSTRACT: This study will see the resurgence of interest in precise velocity dispersion measurements, both for the study of galactic and active nuclei kinematics. As several works suggest, an excellent tactic to measure σ is to use the absorption lines of the calcium triplet, as it is a spectral region relatively free from complications. The discovery of an empirical relationship between the mass of the central black hole (M•) and σ was the leading guide of my detailed study of the calcium triplet region. This search for more accurate methods to calculate the dispersion of velocities, in addition to the careful study of uncertainties. After investing so much time in the development and improvement of the method and its application to so many galaxies, it is time to reap the rewards of this effort, using my results to address a series of questions concerning the physics of galaxies.