This paper is published in Volume-10, Issue-4, 2024
Area
Astrophysics
Author
Arrman Sanganeria
Org/Univ
Independant Researcher, India
Keywords
SPHINX, JWST, Mass, Light, Red-Shift
Citations
IEEE
Arrman Sanganeria. Modelling the Mass to Light Ratios of High Red-Shift Galaxies, International Journal of Advance Research, Ideas and Innovations in Technology, www.IJARIIT.com.
APA
Arrman Sanganeria (2024). Modelling the Mass to Light Ratios of High Red-Shift Galaxies. International Journal of Advance Research, Ideas and Innovations in Technology, 10(4) www.IJARIIT.com.
MLA
Arrman Sanganeria. "Modelling the Mass to Light Ratios of High Red-Shift Galaxies." International Journal of Advance Research, Ideas and Innovations in Technology 10.4 (2024). www.IJARIIT.com.
Arrman Sanganeria. Modelling the Mass to Light Ratios of High Red-Shift Galaxies, International Journal of Advance Research, Ideas and Innovations in Technology, www.IJARIIT.com.
APA
Arrman Sanganeria (2024). Modelling the Mass to Light Ratios of High Red-Shift Galaxies. International Journal of Advance Research, Ideas and Innovations in Technology, 10(4) www.IJARIIT.com.
MLA
Arrman Sanganeria. "Modelling the Mass to Light Ratios of High Red-Shift Galaxies." International Journal of Advance Research, Ideas and Innovations in Technology 10.4 (2024). www.IJARIIT.com.
Abstract
The field of astrophysics is a dynamic and rapidly evolving area of research that seeks to understand the universe's structure, evolution, and fundamental laws governing celestial objects. One of the key areas of interest within astrophysics is the study of galaxy formation and evolution. Galaxies are vast collections of stars, gas, dust, and dark matter held together by gravity, and their formation and evolution processes are crucial for understanding the universe's large-scale structure.