Skip to main content

Research Repository

Advanced Search

Planes of Satellites around Simulated Disk Galaxies. II. Time-persistent Planes of Kinematically Coherent Satellites in ΛCDM

Santos-Santos, Isabel; Gámez-Marín, Matías; Domínguez-Tenreiro, Rosa; Tissera, Patricia B.; Bignone, Lucas; Pedrosa, Susana E.; Artal, Héctor; Gómez-Flechoso, M. Ángeles; Rufo-Pastor, Víctor; Martínez-Serrano, Francisco; Serna, Arturo

Planes of Satellites around Simulated Disk Galaxies. II. Time-persistent Planes of Kinematically Coherent Satellites in ΛCDM Thumbnail


Authors

Matías Gámez-Marín

Rosa Domínguez-Tenreiro

Patricia B. Tissera

Lucas Bignone

Susana E. Pedrosa

Héctor Artal

M. Ángeles Gómez-Flechoso

Víctor Rufo-Pastor

Francisco Martínez-Serrano

Arturo Serna



Abstract

We use two zoom-in ΛCDM hydrodynamical simulations of massive disk galaxies to study the possible existence of fixed satellite groups showing a kinematically coherent behavior across evolution (angular momentum conservation and clustering). We identify three such groups in the two simulations, defining kinematically coherent persistent planes (KPPs) that last at least from virialization to z = 0 (more than 7 Gyr). This proves that orbital pole clustering is not necessarily set in at low redshift, representing a long-lived property of galaxy systems. KPPs are thin and oblate, represent ∼25%–40% of the total number of satellites in the system, and are roughly perpendicular to their corresponding central disk galaxies during certain periods, consistently with Milky Way z = 0 data. KPP satellite members are statistically distinguishable from satellites outside KPPs: they show higher specific orbital angular momenta, orbit more perpendicularly to the central disk galaxy, and have larger pericentric distances than the latter. We numerically prove, for the first time, that KPPs and the best-quality positional planes share the same space configuration across time, such that KPPs act as "skeletons" preventing the latter from being washed out in short timescales. In one of the satellite−host systems, we witness the late capture of a massive dwarf galaxy endowed with its own satellite system, also organized into a KPP configuration prior to its capture. We briefly explore the consequences this event has on the host's KPP and on the possible enhancement of the asymmetry in the number of satellites rotating in one sense or the opposite within the KPP.

Citation

Santos-Santos, I., Gámez-Marín, M., Domínguez-Tenreiro, R., Tissera, P. B., Bignone, L., Pedrosa, S. E., …Serna, A. (2023). Planes of Satellites around Simulated Disk Galaxies. II. Time-persistent Planes of Kinematically Coherent Satellites in ΛCDM. Astrophysical Journal, 942(2), Article 78. https://doi.org/10.3847/1538-4357/aca1c8

Journal Article Type Article
Acceptance Date Nov 2, 2022
Online Publication Date Jan 13, 2023
Publication Date 2023
Deposit Date Jun 8, 2023
Publicly Available Date Jun 8, 2023
Journal Astrophysical Journal
Print ISSN 0004-637X
Electronic ISSN 1538-4357
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 942
Issue 2
Article Number 78
DOI https://doi.org/10.3847/1538-4357/aca1c8
Public URL https://durham-repository.worktribe.com/output/1170426

Files

Published Journal Article (7.5 Mb)
PDF

Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.






You might also like



Downloadable Citations