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Proper Motions of the Satellites of M31

Hodkinson, Ben; Scholtz, Jakub

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Authors

Ben Hodkinson

Jakub Scholtz



Abstract

We predict the range of proper motions of 19 satellite galaxies of M31 that would rotationally stabilize the M31 plane of satellites consisting of 15–20 members as identified by Ibata et al. Our prediction is based purely on the current positions and line-of-sight velocities of these satellites and the assumption that the plane is not a transient feature. These predictions are therefore independent of the current debate about the formation history of this plane. We further comment on the feasibility of measuring these proper motions with future observations by the THEIA satellite mission as well as the currently planned observations by HST and JWST.

Citation

Hodkinson, B., & Scholtz, J. (2019). Proper Motions of the Satellites of M31. Monthly Notices of the Royal Astronomical Society, 488(3), 3231-3237. https://doi.org/10.1093/mnras/stz1893

Journal Article Type Article
Acceptance Date Jul 8, 2019
Online Publication Date Jul 10, 2019
Publication Date Sep 30, 2019
Deposit Date Oct 8, 2019
Publicly Available Date Oct 8, 2019
Journal Monthly Notices of the Royal Astronomical Society
Print ISSN 0035-8711
Electronic ISSN 1365-2966
Publisher Royal Astronomical Society
Peer Reviewed Peer Reviewed
Volume 488
Issue 3
Pages 3231-3237
DOI https://doi.org/10.1093/mnras/stz1893

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Copyright Statement
This article has been accepted for publication in the Monthly notices of the Royal Astronomical Society ©: 2019 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.





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