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• W2029540172 abstract "We present new H i observations of the nearby dwarf galaxy NGC 3741. This galaxy has an extremely extended H i disc, which allows us to trace the rotation curve out to unprecedented distances in terms of the optical disc: we reach 42 B-band exponential scalelengths or about 7 kpc. The H i disc is strongly warped, but the warp is very symmetric. The distribution and kinematics are accurately derived by building model data cubes, which closely reproduce the observations. In order to account for the observed features in the data cube, radial motions of the order of 5–13 km s−1 are needed. They are consistent with an inner bar of several hundreds of pc and accretion of material in the outer regions." @default.
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• W2029540172 date "2007-02-11" @default.
• W2029540172 modified "2023-10-04" @default.
• W2029540172 title "NGC 3741: the dark halo profile from the most extended rotation curve" @default.
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• W2029540172 doi "https://doi.org/10.1111/j.1365-2966.2006.11283.x" @default.
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