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The Pisces Plume and the Magellanic wake

Belokurov, Vasily; Deason, Alis J; Erkal, Denis; Koposov, Sergey E; Carballo-Bello, Julio A; Smith, Martin C; Jethwa, Prashin; Navarrete, Camila

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Authors

Vasily Belokurov

Denis Erkal

Sergey E Koposov

Julio A Carballo-Bello

Martin C Smith

Prashin Jethwa

Camila Navarrete



Abstract

Using RR Lyrae stars in the Gaia Data Release 2 and Pan-STARRS1 we study the properties of the Pisces overdensity, a diffuse substructure in the outer halo of the Milky Way. We show that along the line of sight, Pisces appears as a broad and long plume of stars stretching from 40 to 110 kpc with a steep distance gradient. On the sky Pisces’s elongated shape is aligned with the Magellanic Stream. Using follow-up VLT FORS2 spectroscopy, we have measured the velocity distribution of the Pisces candidate member stars and have shown it to be as broad as that of the Galactic halo but offset to negative velocities. Using a suite of numerical simulations, we demonstrate that the structure has many properties in common with the predicted behaviour of the Magellanic wake, i.e. the Galactic halo overdensity induced by the infall of the Magellanic Clouds.

Citation

Belokurov, V., Deason, A. J., Erkal, D., Koposov, S. E., Carballo-Bello, J. A., Smith, M. C., …Navarrete, C. (2019). The Pisces Plume and the Magellanic wake. Monthly Notices of the Royal Astronomical Society: Letters, 488(1), L47-L52. https://doi.org/10.1093/mnrasl/slz101

Journal Article Type Article
Acceptance Date Jun 21, 2019
Online Publication Date Jun 27, 2019
Publication Date Sep 30, 2019
Deposit Date Sep 13, 2019
Publicly Available Date Sep 13, 2019
Journal Monthly Notices of the Royal Astronomical Society: Letters
Electronic ISSN 1745-3933
Publisher Oxford University Press
Peer Reviewed Peer Reviewed
Volume 488
Issue 1
Pages L47-L52
DOI https://doi.org/10.1093/mnrasl/slz101

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Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society: Letters ©: 2019 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.





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