Cosmological Evolution Effects on the Galactic Size Using Compact Steep Spectrum Sources

Ezeugo Jeremiah Chukwuemerie *

Department of Physics and Industrial Physics, Nnamdi Azikiwe University, Awka, Nigeria.

*Author to whom correspondence should be addressed.


Abstract

Here, we use statistical methods of analyses to find the effects of cosmological evolution on the galactic sizes using compact steep spectrum (CSS) sources. We have done this by carrying out linear regression analysis of observed source linear sizes (D) of CSS quasars against their observed redshifts (z) . Result shows that has an inverse relationship with ; correlation coefficient \((r \approx 0.4)\) is marginal. If is taken to be distance between any two points within a galaxy, this result may be taken to mean cosmological evolution dependence on distance between any two points in an interstellar medium (ISM). In addition, the result of linear size/luminosity \((D-P)\) data indicates that CSS source size shows an inverse power-law function with luminosity. We notice that source luminosity may have a direct link with dynamical evolution; because, it  (P) has been shown to have a direct relationship with source kinetic power. Therefore combining the effects of dynamical evolution and cosmological evolution, we find the relation, \(D \sim P^{-0.16}(1+z)^{-1.52}\). This suggestively implies combined effects of dynamical evolution \(\left(D_{P}\right)\) and cosmological evolution  \(\left(D_{Z}\right)\) on a CSS source size. Finally, we estimate the percentage effects of both  \(\left(D_{P}\right)\) and \(\left(D_{Z}\right)\) on the CSS source size. Results indicate that the effect due to dynamical evolution is ; while that due to cosmological evolution is . From the foregoing, the result obtained for  cosmological evolution simply shows that if is taken to be a distance separating any two positions in any ISM, then the evolution (or expansion) of this distance is appreciable when compared to other forms of evolution. Therefore, we may conclude by stating that as the universe is expanding with time, each galaxy is also expanding in size.

Keywords: Cosmological evolution, linear size, galactic size, luminosity, radio sources, quasars, dynamical evolution, steep spectrum


How to Cite

Chukwuemerie, Ezeugo Jeremiah. 2021. “Cosmological Evolution Effects on the Galactic Size Using Compact Steep Spectrum Sources”. International Astronomy and Astrophysics Research Journal 3 (1):187-92. https://journaliaarj.com/index.php/IAARJ/article/view/52.

Downloads

Download data is not yet available.

References

Ezeugo JC. Jet in the more extended radio sources and unification with compact steep spectrum sources. The Pacific Journal of Science and Technology. 2021;22:14–19.

Ubah OL, Ezeugo JC. Relativistic Jet propagation: Its evolution and linear size cosmic dilation. International Astronomy and Astrophysics Research Journal. 2021;3(3):1–6.

Urry CM. AGN Unification: An Update. Astronomical Society of the Pacific conference series 1; 2004.

Readhead AC. Evolution of powerful extragalactic radio sources. In proc. Colloquium on Quasars and Active Galactic Nuclei, ed. Kohen, M., and Kellermann, K. (USA: National Academy of Sciences, Berkman Center, Irvine). 1995;92:11447–11450.

Robson I. Active galactic nuclei, John Wiley and Sons Ltd, England; 1996.

Jackson JC. Radio source evolution and unified schemes. Publications of Astronomical Society of the Pacific. 1999; 16:124–129.

Kawakatu N, Kino M. The velocity of large-scale jets in a declining density medium. In Serie de Conferencias. Triggering Relativistic Jets, ed. W.H. Lee and E. Ramirez-Ruiz. 2007;27:192–197.

Mahatma VH, Hardcastleand MJ, Williams WL. LoTSS DR1: Double-double radio galaxies in the HETDEX field. Astronomy and Astrophysics. 2019;622:A13.

Mingo B, Croston JH, Hardcastle MJ. Revisiting the fanaroff-riley dichotomy and radio galaxy morphology with the LOFAR two-meter sky survey (LoTSS). Monthly Notices of the Royal Astronomical Society. 2019;488:2701–2721.

Hardcastle WL, Williams WL, Best PN. Radio-loud AGN in the first LoTSS data release — The lifetimes and environmental impact of jet-driven sources. Astronomy and Astrophysics. 2019;622:A12.

Dabhade P, Gaikwad M, Bagchi J. Discovery of giant radio galaxies from NVSS: Radio and infrared properties. Monthly Notices of the Royal Astronomical Society. 2017;469(3):2886–2906.

Ezeugo JC, Ubachukwu AA. The spectral turnover–linear size relation and the dynamical evolution of compact steep spectrum sources. Monthly Notices of the Royal Astronomical Society. 2010;408: 2256–2260.

O’Dea CP. The compact steep spectrum and gigahertz peaked spectrum radio sources. Publications of the Astronomical Society of the Pacific. 1998;110:493– 532.

Fanti C, Fanti R, Dallacasa D, Schillizzi RT, Spencer RE, Stanghellini C. Are compact steep spectrum sources young? Astronomy and Astrophysics. 1995; 302:317–326.

Ezeugo JC. On the intergalactic media densities, dynamical ages of some powerful radio sources and implications. Journal of Physical Sciences and Application. 2021;11(1):29–34.

Ezeugo JC. Compact spectrum source size and cosmological implication. Journal of Research in Applied Mathematics. 2021; 7(2):1–4.

Ezeugo JC. Compact steep-spectrum radio sources and ambient medium density. International Journal of Astrophysics and Space Science. 2015; 3(1):1–6.

Ezeugo JC. On the dependence of spectral turnover on linear size of compact steep-spectrum radio sources. International Journal of Astrophysics and Space Science. 2015;3(2):20–24.

Ezeugo JC. On cosmic epoch and linear size/luminosity evolution of compact steep spectrum sources. American Journal of Astronomy and Astrophysics. 2021;9(1): 8–12.