Deep DRAO HI observations of the Local Group BCD IC 10 confirm a faint NW hydrogen cloud, yield a steep inner rotation curve, and indicate the inner disk can be modeled without dark matter, while simulations disfavor an M31 interaction as the source of the galaxy's disturbed HI.
G., Johnson M., Nidever D
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HI observations of IC 10 with the DRAO synthesis telescope
Deep DRAO HI observations of the Local Group BCD IC 10 confirm a faint NW hydrogen cloud, yield a steep inner rotation curve, and indicate the inner disk can be modeled without dark matter, while simulations disfavor an M31 interaction as the source of the galaxy's disturbed HI.