International Journal of Astronomy
p-ISSN: 2169-8848 e-ISSN: 2169-8856
2021; 10(1): 6-12
doi:10.5923/j.astronomy.20211001.02
Received: Feb. 9, 2021; Accepted: Mar. 9, 2021; Published: Mar. 20, 2021

Adrián G. Cornejo
Electronics and Communications Engineering from Universidad Iberoamericana, Santa Rosa 719, Querétaro, Mexico
Correspondence to: Adrián G. Cornejo , Electronics and Communications Engineering from Universidad Iberoamericana, Santa Rosa 719, Querétaro, Mexico.
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Copyright © 2021 The Author(s). Published by Scientific & Academic Publishing.
This work is licensed under the Creative Commons Attribution International License (CC BY).
http://creativecommons.org/licenses/by/4.0/

This work describes the hypothesis in which the explanation of the rotational velocity of barred spiral galaxies is based on the relativistic solution. Considering a previous relativistic solution for the unbarred spiral galaxies, this solution assumes that the entire spiral galaxy disk would rotate like a rigid (or solid) body. It is considered that both the Solar System and spiral galaxies are behaving like a rigid body in rotation. Then, having both systems the same dynamical behaviour, which can be explained by the same relativistic solution, these two apparently different cases are unified in the same solution. Thus, the stars and gas in the spiral galaxy must be rotating with the system in an almost the same and uniform angular velocity. Nevertheless, according to the Kerr metric for the rotating black hole, at the zone of the bar of barred spiral galaxies, stars and gas must be changing their direction toward the rotation poles of the black hole. On these assumptions, we apply the equation based on the relativistic solution to the barred spiral galaxies. More precisely, we present examples of the rotation curves of unbarred spiral galaxies: NGC 4378 and NGC 4594, and the barred spiral galaxies: Milky Way and, NGC 7541. Comparing our calculations with the observations we find a good approximation.
Keywords: Galaxies: spiral, Kinematics and dynamics, General Theory of Relativity
Cite this paper: Adrián G. Cornejo , The Rotational Velocity of Barred Spiral Galaxies in the General Relativity Solution, International Journal of Astronomy, Vol. 10 No. 1, 2021, pp. 6-12. doi: 10.5923/j.astronomy.20211001.02.
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![]() | Figure 1. Kerr metric of a rotating black hole |
![]() | Figure 2. The dynamics around the Kerr metric of a rotating black hole, and the forming of the bar of a barred spiral galaxy |
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