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This document summarizes a study examining dwarf galaxies at the steep, faint end of the Tully-Fisher relation. The study claims that the properties of dwarf galaxies, such as their rotation curves, radial acceleration relations, and positions on the Tully-Fisher relation, can be explained by considering that dwarf galaxies orbiting larger host galaxies are immersed in a slightly warmer thermal bath than isolated dwarf galaxies due to radiation from their hosts. The study finds that when accounting for this

Author

michele

Language

EN