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- W2114598219 abstract "We study the vertical gradient in azimuthal velocity of spiral galaxy NGC 4244 in a thin disk model. With surface density accounting for the rotation curve, we model the gradient properties in the approximation of quasi-circular orbits and find the predictions to be consistent with the gradient properties inferred from measurements. This consistency may suggest that the mass distribution in this galaxy is flattened." @default.
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- W2114598219 date "2015-06-24" @default.
- W2114598219 modified "2023-10-16" @default.
- W2114598219 title "Modelling vertical structure in circular velocity of spiral galaxy NGC 4244" @default.
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- W2114598219 doi "https://doi.org/10.1093/mnras/stv1163" @default.
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