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Article
Formation of ultra-diffuse galaxies in the field and in galaxy groups
Monthly Notices of the Royal Astronomical Society (2019)
  • Fangzhou Jiang, The Hebrew University
  • Avishai Dekel, The Hebrew University
  • Jonathan Freundlich, The Hebrew University
  • Aaron J. Romanowsky, San Jose State University
  • Aaron A. Dutton, New York University Abu Dhabi
  • Andrea V. Macciò, New York University Abu Dhabi
  • Arianna Di Cintio, Institute of Astrophysics of the Canary Islands
Abstract
We study ultra-diffuse galaxies (UDGs) in zoom in cosmological simulations, seeking the origin of UDGs in the field versus galaxy groups. We find that while field UDGs arise from dwarfs in a characteristic mass range by multiple episodes of supernova feedback (Di Cintio et al.), group UDGs may also form by tidal puffing up and they become quiescent by ram-pressure stripping. The field and group UDGs share similar properties, independent of distance from the group centre. Their dark-matter haloes have ordinary spin parameters and centrally dominant dark-matter cores. Their stellar components tend to have a prolate shape with a Sérsic index n ∼ 1 but no significant rotation. Ram pressure removes the gas from the group UDGs when they are at pericentre, quenching star formation in them and making them redder. This generates a colour/star-formation-rate gradient with distance from the centre of the dense environment, as observed in clusters. We find that ∼20 per cent of the field UDGs that fall into a massive halo survive as satellite UDGs. In addition, normal field dwarfs on highly eccentric orbits can become UDGs near pericentre due to tidal puffing up, contributing about half of the group-UDG population. We interpret our findings using simple toy models, showing that gas stripping is mostly due to ram pressure rather than tides. We estimate that the energy deposited by tides in the bound component of a satellite over one orbit can cause significant puffing up provided that the orbit is sufficiently eccentric. We caution that while the simulations produce UDGs that match the observations, they under-produce the more compact dwarfs in the same mass range, possibly because of the high threshold for star formation or the strong feedback.
Keywords
  • galaxies: evolution,
  • galaxies: formation,
  • galaxies: haloes
Publication Date
August, 2019
DOI
10.1093/mnras/stz1499
Publisher Statement
This article has been accepted for publication in 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. This article can also be found online at the following link: https://doi.org/10.1093/mnras/stz1499

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Citation Information
Fangzhou Jiang, Avishai Dekel, Jonathan Freundlich, Aaron J. Romanowsky, et al.. "Formation of ultra-diffuse galaxies in the field and in galaxy groups" Monthly Notices of the Royal Astronomical Society Vol. 487 Iss. 4 (2019) p. 5272 - 5290 ISSN: 00358711
Available at: http://works.bepress.com/aaron_romanowsky/160/