The proper motion of the Local Group galaxy IC 10

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Abstract
We have measured the proper motion of the Local Group galaxy IC 10 with the Very Long Baseline Array by measuring the position of an H2O maser relative to two background quasars over 4.3 years. After correction for the rotation of the Milky Way and IC 10, we obtain a motion of – μas yr-1 toward the East and μas yr-1 toward the North. This corresponds to a total space velocity of km s-1 relative to the Milky Way for an assumed distance of kpc. Assuming that IC 10 and M 33, for which also a proper motion measurement exists, are bound to M 31, we calculate a lower limit for the mass of M 31 of .
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