Dark Matter in the Central Region of NGC 3256

Abstract

We investigated the central mass distribution of the luminous infrared galaxy NGC 3256 at a distance of 35 Mpc by using

Dark matter effect attributed to the inherent structure of cosmic space

“…Using this simple modification to the Gravity Law, MOND has been successful in explaining the dark matter effect for a great majority of observations. 15 However, there have also been notable outliers, such as galaxies appearing to have too little 16 or too much 17 dark matter to fit into MOND's simple one-parameter model. Randriamampandry and Carignan 18 show that among a sample of fifteen galaxies, six do not fit well MOND if a 0 were treated as a universal constant but prefer larger or smaller values for it compared to the one given in Equation (1.1).…”