Formation of ultra-diffuse galaxies in the field and in galaxy groups

Fangzhou Jiang, Avishai Dekel, Jonathan Freundlich, Aaron J. Romanowsky, Aaron A. Dutton, Andrea Maccio, Arianna Di Cintio

Research output: Contribution to journalArticle

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.

Original languageEnglish (US)
Article numberstz1499
Pages (from-to)5272-5290
Number of pages19
JournalMonthly Notices of the Royal Astronomical Society
Volume487
Issue number4
DOIs
StatePublished - Jun 25 2019

Fingerprint

galactic clusters
galaxies
tide
ram
gas
simulation
tides
stripping
star formation
halos
dark matter
energy
orbits
eccentric orbits
eccentrics
star formation rate
gases
supernovae
quenching

Keywords

  • galaxies: evolution
  • galaxies: formation
  • galaxies: haloes

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Jiang, F., Dekel, A., Freundlich, J., Romanowsky, A. J., Dutton, A. A., Maccio, A., & Di Cintio, A. (2019). Formation of ultra-diffuse galaxies in the field and in galaxy groups. Monthly Notices of the Royal Astronomical Society, 487(4), 5272-5290. [stz1499]. https://doi.org/10.1093/mnras/stz1499

Formation of ultra-diffuse galaxies in the field and in galaxy groups. / Jiang, Fangzhou; Dekel, Avishai; Freundlich, Jonathan; Romanowsky, Aaron J.; Dutton, Aaron A.; Maccio, Andrea; Di Cintio, Arianna.

In: Monthly Notices of the Royal Astronomical Society, Vol. 487, No. 4, stz1499, 25.06.2019, p. 5272-5290.

Research output: Contribution to journalArticle

Jiang, F, Dekel, A, Freundlich, J, Romanowsky, AJ, Dutton, AA, Maccio, A & Di Cintio, A 2019, 'Formation of ultra-diffuse galaxies in the field and in galaxy groups', Monthly Notices of the Royal Astronomical Society, vol. 487, no. 4, stz1499, pp. 5272-5290. https://doi.org/10.1093/mnras/stz1499
Jiang, Fangzhou ; Dekel, Avishai ; Freundlich, Jonathan ; Romanowsky, Aaron J. ; Dutton, Aaron A. ; Maccio, Andrea ; Di Cintio, Arianna. / Formation of ultra-diffuse galaxies in the field and in galaxy groups. In: Monthly Notices of the Royal Astronomical Society. 2019 ; Vol. 487, No. 4. pp. 5272-5290.
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