The proper motion of Andromeda from Gaia eDR3: confirming a nearly radial orbit
J.-B. Salomon, R. Ibata, C. Reyl\'e, B. Famaey, N. I. Libeskind, A.W., McConnachie, Y. Hoffman

TL;DR
This study measures Andromeda's proper motion using Gaia eDR3 data, confirming a nearly radial orbit and providing more precise velocity estimates that support future galaxy merger predictions.
Contribution
The paper presents the first Gaia-based proper motion measurement of Andromeda, refining previous estimates and analyzing stellar population differences within M31.
Findings
Proper motion of M31 measured at 52.5 +/- 5.8 muas/yr
Relative velocity between M31 and Milky Way is 42.2 +/- 39.3 km/s
Transverse velocity of M31 is 82.4 +/- 31.2 km/s
Abstract
We present an analysis of the proper motion of the Andromeda galaxy (M31), based on the Early Third Data Release of the Gaia mission. We use the Gaia photometry to select young blue main sequence stars, and apply several quality cuts to obtain clean samples of these tracers. After correcting the proper motion measurements for the internal rotation of the M31 disk motion, we derive an apparent motion of 52.5 +/- 5.8 muas/yr with respect to the Gaia reference frame, or 61.9 +/- 9.7 muas/yr after applying a zero-point correction determined from quasars within 20 degrees from M31 and a correction from systemic biases. Accounting for the Solar reflex motion we deduce a relative velocity between Andromeda and the Milky way (in a non-rotating frame at the current location of the Sun) of 42.2 +/- 39.3 km/s along right ascension (40.0 +/- 39.3 km/s along galactic longitude) and -59.4 +/- 30.3…
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