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This paper introduces an anisotropic generalization of the semi-isotropic axisymmetric Jeans formalism to model the stellar kinematics of galaxies, focusing on fast-rotator early-type galaxies. The method, which requires only two free parameters, effectively describes the velocity moments and can recover the inclination and mass-to-light ratio of galaxies, while allowing for the inclusion of dark matter and other complexities. The findings are validated against integral-field observations, demonstrating the

Author
Phan Quốc Việt Anh
Language
EN