Distribution of Galaxies' Brightness for Spheroidal Distribution Models of Luminosity and Absorbing Matter
Abstract
Distribution of luminosity in galaxies is of no small importance for clarifying the physical processes that occur therein. The observed distribution is described by the surface brightness, which is the projection of luminosity on the perspective plane along the line of sight.
Published
2020-05-20
How to Cite
Maria A. Mardanova. (2020). Distribution of Galaxies’ Brightness for Spheroidal Distribution Models of Luminosity and Absorbing Matter. International Journal of Advanced Science and Technology, 29(7), 1813 - 1820. Retrieved from http://sersc.org/journals/index.php/IJAST/article/view/17073
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Articles